The galaxy appears to be an elliptical type, exhibiting a generally smooth, symmetrical morphology. It displays a concentrated central bulge, which fades into a diffuse halo. The color profile suggests an older stellar population, with a yellowish-red hue dominating, and a slightly bluer tint further from the galactic center. There is a slight suggestion of an elliptical shape and the galaxy does not display any strong signs of spiral arms or significant dust lanes. There are no visible signs of tidal disturbances or ongoing major merger activity, although a subtle asymmetry may indicate a minor interaction in the past. The overall impression is of a relatively quiescent system.
