The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light profile. It's elongated, with a shape that is slightly more elongated than a perfectly round system. The core exhibits a brighter, more concentrated luminosity, suggesting a significant accumulation of older stellar populations. There is a subtle color gradient apparent, with a slightly bluer hue toward the outer regions and a redder hue towards the core. This could suggest ongoing, albeit modest, star formation activity in the outer regions, whereas the central bulge likely consists of older, redder stars. The overall structure lacks any prominent spiral arms or dust lanes. There are signs of minor disturbances that could be due to gravitational interactions with another galaxy.
