The galaxy presents an elongated, cigar-shaped morphology, suggesting a likely classification as an elliptical galaxy or a lenticular galaxy viewed edge-on. It exhibits a central bulge that appears relatively bright and concentrated, transitioning to a fainter and more diffuse outer disk or halo. The light distribution indicates a primarily older stellar population, with the yellowish-orange hue dominating the central region, indicative of lower star formation rates. There's a subtle hint of bluer light distributed within the disk or outer regions, suggesting the presence of some younger, hotter stars, though this is not dominant. The overall smooth appearance indicates that it is unlikely to be undergoing any major mergers, though the overall asymmetrical light distribution indicates minor disturbances may have occurred in the recent past. No distinct spiral arms are discernible in the image.
