The galaxy presents as a moderately luminous, elliptical or lenticular system, exhibiting a notable red-yellow color profile. The central region is characterized by a bright, concentrated bulge, suggestive of an older stellar population. There appears to be a faint, diffuse disk component. The galaxy's overall structure is relatively smooth, with no obvious signs of active star formation regions or spiral arm structures. The shape is somewhat elongated and cigar shaped, but generally smooth, which suggests that it may be in the process of evolving into a more elliptical form. There is no obvious evidence of tidal tails, mergers, or major disturbances affecting the galaxy's morphology. The galaxy appears to be relatively isolated.