The galaxy presents a generally elliptical morphology. The light distribution appears relatively smooth, lacking prominent spiral arms or significant dust lanes. The central region exhibits a bright, concentrated core, suggesting a high stellar density or potentially an active galactic nucleus. The galaxy displays a color gradient, transitioning from a more reddish hue in the central region to a bluer color in the outer regions. This color difference could indicate an older stellar population in the core and younger stars in the outer disk, suggestive of ongoing or recent star formation. There is no evidence of major tidal disturbances or ongoing mergers, although minor irregularities may be present in the outer halo.
