The galaxy presents as a largely featureless elliptical or lenticular system. It exhibits a smooth, diffuse morphology with a centrally concentrated brightness profile, indicative of an older stellar population. A prominent, luminous bulge dominates the visual appearance, gradually fading into a less distinct halo. The overall color appears to be on the redder end, consistent with a population of evolved stars and suggesting limited ongoing star formation. No spiral arm structures or dust lanes are clearly visible. There may be some faint, diffuse outer regions but the data resolution limits a detailed characterization. There is no sign of major mergers or major disturbances.
