The galaxy presents a generally elliptical morphology, with a smooth, diffuse appearance. Its light profile seems to transition gradually from the central region outwards, showing no distinct spiral arm structures or sharp boundaries. The core region exhibits a concentrated luminosity, suggesting a higher density of stars or a possible active galactic nucleus, though no clear jet or point source is visible within the image. A subtle color gradient can be observed, with the central regions appearing slightly more yellow or red, and the outer regions displaying a bluer tint. This may indicate a difference in stellar populations, with older, redder stars concentrated toward the center and younger, bluer stars in the outskirts. There appears to be a slight asymmetry, possibly due to tidal interactions or an ongoing minor merger event, but the evidence is not definitive from this image alone. The overall structure seems relatively undisturbed, without major distortions or prominent tidal tails, implying that the galaxy is likely not undergoing a significant merger. The galaxy is modestly sized, neither exceptionally large nor remarkably compact.
