The galaxy presents a moderately elliptical morphology, appearing somewhat cigar-shaped in its overall form. It exhibits a diffuse, smooth light distribution with a possible faint disk-like structure. The central region appears slightly more concentrated in brightness, indicative of a nucleus or bulge. There are no discernible spiral arms or prominent dust lanes visible in this image. The color appears to be generally redder, suggesting a population dominated by older stars and/or a significant presence of dust within the galaxy. There is potential evidence of minor disturbances, possibly related to a past or ongoing interaction, although no clear merger features are immediately apparent. The galaxy is relatively compact in size.
