The galaxy appears as a centrally concentrated object with a generally smooth morphology. The light profile suggests a possible elliptical galaxy, or perhaps a spiral viewed face-on with limited visible spiral arm structure. The central region exhibits a higher surface brightness, with the luminosity gradually decreasing outwards towards its edges. The shape deviates slightly from perfectly circular, exhibiting a mild elongation, but is mostly categorized as moderately rounded. There is no obvious presence of tidal tails, merging companions, or strong asymmetries suggestive of recent major merger events. The galaxy exhibits a redder color in its core, transitioning to slightly bluer hues in the outer regions. This color gradient may imply an older stellar population concentrated in the central bulge, with younger stars contributing to the bluer light observed further from the center where star formation may be occurring.
