The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its shape appears to be elliptical, though it is difficult to discern any fine details or spiral structure due to its relative distance and apparent lack of distinct features. The light distribution within the galaxy gradually fades from a bright central region outwards, with no sharp edges or clearly defined spiral arms visible. The color profile suggests an older stellar population, with a somewhat reddish hue indicative of relatively low levels of current star formation. There is no obvious evidence of ongoing major mergers or tidal disturbances, which, along with its smooth appearance, point towards a relaxed and relatively undisturbed evolutionary state.
