The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a bright, concentrated core with a yellowish hue, suggestive of an older stellar population. Moving outward from the core, the color transitions to a slightly bluer shade, indicating the presence of some younger stars. The overall form is slightly elongated, departing somewhat from a perfect circle, but is primarily spheroid in nature. There are no apparent spiral arms, bars, or other distinct features indicative of a disk galaxy. Faint, diffuse light extends outwards from the central region, gradually fading into the background. There is no evidence of any major ongoing merger activity or significant tidal disturbances. It is possible there could be minor disturbances but it is hard to say.
