The galaxy presents a moderately luminous profile, appearing as a single core. There is a small, lower luminosity, nearby feature that may represent a satellite galaxy or tidal debris. The main galaxy's overall structure indicates a relatively smooth, possibly elliptical morphology. The light distribution suggests it is mostly uniform with minimal complex substructure. Color analysis reveals a population of older stars dominating the emission, as indicated by the shift towards redder wavelengths. The morphology appears to be dominated by a spheroid. The small feature seems more point-like and may be experiencing mild tidal disruption.
