The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. While the overall structure appears mostly undisturbed, there is evidence of possible tidal interactions or a merger event. The galaxy's light profile suggests an older stellar population, with the core exhibiting a more reddish hue. A faint, extended halo is suspected, although the low resolution hinders precise determination of its boundaries. The redder colors are typical of older stellar populations that have largely ceased star formation. 
