The galaxy presents an overall elliptical morphology, appearing largely smooth and spheroidal in shape. A pronounced central bulge is evident, exhibiting a concentrated luminosity that decreases gradually towards the outer regions. The galaxy exhibits a color gradient, with the core showing a yellowish hue, suggestive of an older stellar population. This color shifts toward a slightly bluer tint within the surrounding halo. There is no obvious presence of strong spiral arm structures or significant dust lanes. Faint wisps of light extend outwards, indicating possible tidal features, however no significant merging events or major disturbances are directly observable. Overall, the galaxy appears to be a relatively undisturbed system.