The galaxy presents as a single, largely featureless entity, exhibiting a smooth and rounded morphology. There is no clear evidence of spiral arm structure or a distinct central bulge. The light profile appears concentrated towards the center, suggesting a centrally dominant stellar population. The color index indicates that the galaxy appears relatively red, potentially implying a population of older stars. The absence of prominent blue regions suggests a low ongoing star formation rate. There is no obvious indication of recent or ongoing merger activity, with no tidal tails or significant morphological distortions visible. The galaxy is likely an elliptical or S0 type galaxy.
