The galaxy appears as a single, relatively smooth elliptical system, characterized by a concentrated central bulge and a diffuse halo. There is a slight elongation of the galaxy, suggesting a deviation from perfect sphericity, more towards a slightly oblate spheroid. The color profile indicates a dominant older stellar population, signified by the reddish-yellow hue. There is no obvious evidence of distinct spiral arm structures or active star-forming regions based on the lack of blue light. There may be some disruption in form, possibly indicating that this galaxy is in the process of merging with another, or has undergone a minor disturbance. Overall, the galaxy appears relatively undisturbed.
