The galaxy presents as an elliptical structure, with a generally smooth appearance. It is elongated, appearing cigar-shaped. The galaxy exhibits a dominant central bulge, which appears to be a concentrated region of luminosity. The overall color profile suggests a moderate redshift. There are hints of underlying disk-like structures; however, they are largely obscured by the pronounced bulge and smooth overall morphology. No major mergers or strong tidal features are evident, although there is a slight asymmetry which might indicate a recent, minor interaction. The stellar population likely consists primarily of older stars, which are more concentrated in the central region.
