The galaxy presents as a single, mostly unresolved object. It exhibits a smooth, elliptical morphology with a high degree of circularity. The light distribution is concentrated towards the center, gradually decreasing in intensity outwards with no obvious signs of distinct features or substructure. The galaxy's color profile is dominated by redder wavelengths, indicating a population of older stars and a relatively low rate of ongoing star formation. There is no evidence of a prominent disk, spiral arms, or recent merger activity. The galaxy appears quiescent and evolved.
