The galaxy presents as a fairly well-defined elliptical morphology. The light distribution appears generally smooth, with a concentration towards the central region, indicating a prominent bulge. There is little evidence of distinct spiral arms or a well-defined disk structure. The galaxy exhibits a bluer color profile, suggestive of ongoing star formation, though the overall smooth appearance hints at a relatively evolved stellar population. There may be a slight indication of tidal features, though they do not appear prominent and may result from minor interaction or merger. The overall structure indicates a mass in the typical galaxy range and a moderate rate of star formation.
