The galaxy presents a somewhat amorphous structure with a dominant, centrally concentrated luminosity profile. It exhibits a slightly elongated shape, deviating marginally from a perfect circle. Within the brighter central region, subtle variations in color suggest the presence of distinct stellar populations. While the galaxy appears mostly smooth, there are hints of faint, diffuse features extending outwards, possibly indicating tidal interactions or minor disturbances. Overall, the galaxy displays an intermediate color, exhibiting a modest level of star formation. Evidence suggests there might be a past or ongoing interaction with another galaxy. The overall structure is suggestive of a system undergoing transition in its morphological type.
