The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. A prominent, bright bulge dominates the central region, fading gradually into a less luminous, diffuse halo. There's little evidence of spiral arm structure or significant dust lanes. The overall color appears relatively uniform with hints of a yellow/red hue, suggesting an older stellar population. A slight deviation from perfect circularity is observed, with the galaxy appearing somewhat flattened. There are no clear signs of tidal disturbances or interactions with neighboring galaxies, although a minor asymmetry in the outer halo can not be discounted. The galaxy does not appear to be actively undergoing a major merging event.
