The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that transitions outwards to a more diffuse halo. The color profile indicates a dominant population of older stars, with a yellowish-red hue. The galaxy appears to be relatively isolated with no obvious signs of tidal disruption or recent merger events. There is a very slight elongation, not quite fully spherical, tending towards an intermediate roundedness. There are no visually prominent dust lanes or spiral arm structures. Overall, the galaxy exhibits characteristics consistent with a well-evolved, relatively quiescent system.
