The galaxy presents a smooth, somewhat elongated morphology. Its color profile suggests an evolved stellar population, appearing primarily yellowish-orange with a subtle concentration towards the center, suggestive of an older core population. No prominent spiral arm structures or dust lanes are discernible. The galaxy exhibits a moderately compact size. There's no readily apparent evidence of ongoing major merger activity or significant tidal disturbances, though there's a hint of a minor asymmetry. The relatively uniform color distribution and lack of distinct features suggest that this galaxy is a relatively quiescent system.
