The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light profile appears uniform, decreasing gradually from the bright core to the outer regions, showing limited evidence of spiral arms or significant dust lanes. The color appears to be shifted towards the redder end of the spectrum, suggesting a population dominated by older stars. The galaxy appears generally undisturbed, although it is challenging to determine if there may be any faint tidal features indicative of past interactions.
