The galaxy presents as a centrally concentrated, relatively smooth object. The core region exhibits a bright, diffuse glow, suggesting a high density of stars or active galactic nucleus activity. Moving outwards from the core, the light intensity gradually diminishes, with a transition to less luminous, more mottled features in the outer regions. The overall shape of the galaxy approximates a somewhat elliptical morphology, deviating slightly from a perfectly circular form. There are some hints of substructure in the outer regions, but the light is not evenly distributed, indicating some minor asymmetries or potential tidal effects. The galaxy appears to be relatively undisturbed, with no obvious signs of a recent major merger or strong tidal interaction. The colors suggest a mixed stellar population, with a relatively redder core implying older stars and potentially more dust, with slightly bluer colors in the surrounding area.
