The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. It exhibits a yellowish-orange hue, indicative of a stellar population that is likely older and contains fewer young, hot stars. There's little evidence of distinct spiral arms or prominent dust lanes, suggesting a morphology closer to an elliptical galaxy or a lenticular galaxy viewed face-on. The galaxy displays a high degree of central concentration. There is no visible sign of any major merging activity, and the overall shape is quite regular, with minimal disturbance apparent in the image. A very faint, diffuse halo is suspected, extending slightly beyond the main body of the galaxy.
