This galaxy presents as a relatively smooth, elliptical structure with a centrally concentrated luminosity profile. The light distribution is dominated by older stellar populations, inferred from the redder color indices. There is little evidence of spiral arms or significant dust lanes, suggesting a lack of recent major star formation events. The object appears nearly round in projection, with minimal apparent ellipticity. There is no readily apparent tidal features or close companion galaxies, indicating it has likely undergone no recent major merger events. The galaxy's light profile fades gradually into the surrounding background sky. The relatively compact size and lack of significant star formation suggests the galaxy is a quiescent system.
