This galaxy presents as a relatively smooth object with a concentrated central bulge. It appears somewhat elliptical in shape, tending towards a more spheroidal morphology rather than a flattened disk structure. The galaxy's color profile suggests an older stellar population, with light trending towards the redder end of the spectrum. There is minimal evidence of ongoing star formation or distinct spiral arm features. Subtle disturbances in its shape suggest the possibility of a minor interaction or past merger event. Its overall structure indicates a well-evolved system, likely dominated by older stars and with a considerable mass.
