The galaxy presents as a relatively smooth, centrally concentrated object with a nearly circular morphology. There is a slight elongation to the overall structure but no discernible spiral arm features. The color profile indicates a somewhat redder core, surrounded by a slightly bluer outer region. The overall color suggests a population of older stars, with some evidence of on-going but relatively low-level star formation. There are no clear signs of major mergers or tidal disturbances, although there is some slight asymmetry in the overall distribution of light, suggesting possible minor interactions. The galaxy appears to be relatively isolated, with no immediately obvious companion galaxies.
