The galaxy presents a generally elliptical morphology, elongated along a primary axis. The light distribution appears centrally concentrated with a smooth profile, suggesting a relatively evolved stellar population. The core exhibits a yellowish hue, potentially indicative of older, redder stars dominating the central region. Fainter, bluer light is observed in regions extending away from the core, hinting at the presence of younger stars and/or ongoing star formation, albeit at a low rate. There is evidence of a possible minor tidal disturbance.
