The galaxy presents as a spheroid with a dominant, smooth central bulge. The light distribution is centrally concentrated, diminishing outwards in a gradient fashion. The colour of the bulge appears yellowish-orange, potentially indicating an older stellar population with a lower rate of ongoing star formation. The galaxy exhibits minimal discernible disk structure, suggesting a classification leaning towards elliptical. Subtle distortions in the outer regions may point to minor gravitational interactions, or could simply be irregularities in the galaxy's halo structure. There are no clear signs of any active galactic nucleus activity. Overall, the galaxy appears to be relatively isolated and quiescent.
