The galaxy appears as a fairly smooth, elliptical-like structure with a centrally concentrated brightness profile. It exhibits a yellowish hue, suggesting a population of older stars. There is a slight elongation, but overall, it is relatively round. No distinct spiral arms or prominent dust lanes are visible. The galaxy shows no signs of major tidal disturbances or ongoing mergers; it seems to be a relatively undisturbed system. There is some blueish tint in areas of the disk possibly indicating star formation or possibly be background noise.
