The galaxy presents as a relatively compact structure, appearing generally smooth in texture. The core region displays a concentrated luminosity, suggesting a higher density of stellar populations or perhaps the presence of an active galactic nucleus, though the image resolution limits definitive identification. The overall morphology seems elliptical, with a high degree of circularity. There are subtle variations in color across the galaxy, transitioning from bluer hues in one apparent region to more yellow-red tones across the other portions of the galaxy. There is no obvious spiral arm structure or significant dust lane obscuration visible. The galaxy does not appear to be undergoing any major merging activity or possess any tidal tails, implying it is in a relatively quiescent state dynamically.
