The galaxy presents as a centrally concentrated object with a generally smooth morphology, suggesting a lack of significant spiral arm structure or strong irregularities. The light profile is relatively smooth. The central region appears to be dominated by older stellar populations, indicated by its yellowish color. There is some evidence of a possible tidal feature or minor interaction occurring near the galaxy, given its asymmetry and the presence of a possible secondary nucleus or bright knot located close to it. This could indicate a minor disturbance or recent merger event, although the main body of the galaxy appears largely undisturbed. The object is relatively compact, consistent with a moderate physical size at its estimated distance. There is some indication of ongoing or recent star formation, as traced by slightly bluer regions outside the center, although the overall color profile is dominated by redder light, suggesting that star formation rates are relatively low. There is little to no indication of significant dust extinction within the galaxy.
