The galaxy presents as a concentrated, centrally bright object, appearing largely smooth in texture with little to no discernible spiral arm structure. It has a generally round morphology, with a slight elongation.  There appears to be a faint, diffuse halo extending beyond the central region. The color profile suggests a population of older stars dominating the light output, and the low star formation rate is consistent with this assessment. There is no strong evidence of a major merger event or significant tidal disturbances in its immediate vicinity.
