The galaxy presents as a well-defined, elliptical structure. The central region exhibits a concentrated luminosity, appearing almost spheroidal and smooth. Moving outward from the core, the light gradually decreases. The overall color profile suggests a predominantly older stellar population. There's minimal evidence of spiral arm structures or significant dust lanes. Faint tidal features appear to be present, suggesting a past or ongoing interaction, though not a major merger event. The isophotes are largely concentric.
