The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light profile. The central region is characterized by a bright, concentrated core, suggesting a significant stellar density. The overall color appears to be a yellow-orange hue, potentially indicative of an older stellar population dominated by redder stars and a relative lack of ongoing star formation. The galaxy appears elongated, with a cigar-like shape, indicating a non-spherical distribution of its constituent stars. There's no clear evidence of spiral arms or significant dust lanes, and there is an apparent lack of tidal features, suggesting a relatively undisturbed evolutionary history without recent major mergers.
