The galaxy exhibits a largely smooth, elliptical morphology. It appears nearly circular in projection, with minimal deviation from a rounded shape. There is a concentration of light towards the galaxy's center, suggesting a prominent galactic bulge. A slight color gradient is observed, with the central region appearing more yellowish-orange, possibly indicating an older stellar population. Fainter, bluer regions extend outward from the center, potentially signifying areas of more recent star formation, although star formation is relatively low. There is no apparent presence of spiral arms or a distinct disk structure. No significant signs of tidal disturbances or interactions with other galaxies are visible, indicating it is likely an isolated system at its current evolutionary stage.
