The galaxy appears as a centrally concentrated, relatively smooth structure with a generally elliptical morphology. The core region exhibits a bright, concentrated luminosity. There is a falloff in luminosity extending outwards from the core, lacking distinct spiral arms or a pronounced disk-like structure. The color profile exhibits subtle variations, with a slight blue tint becoming more prominent in the outer regions suggesting a small degree of on-going star formation. There appears to be minimal evidence of significant tidal disruption or ongoing merger events.
