The galaxy presents a generally smooth and featureless appearance. Its morphology seems predominantly elliptical or lenticular, characterized by a centrally concentrated luminosity profile. There is a significant spheroidal component, as indicated by the rounded shape. The galaxy exhibits a yellowish-red hue, suggestive of an older stellar population and a relative lack of ongoing star formation. No prominent spiral arms or distinct dust lanes are discernible. Faint, diffuse extensions are potentially present, though these are subtle and do not indicate any major ongoing merger events. The galaxy seems isolated, with no obvious tidal interactions or nearby companion galaxies.
