The galaxy presents as an elliptical or lenticular type, characterized by a relatively smooth, diffuse light distribution. The overall shape is elongated, exhibiting a moderate cigar-shaped appearance. There appears to be no significant presence of spiral arms or a prominent disk structure; the galaxy is mostly spheroid. There may be subtle irregularities in its morphology, which could be a sign of a prior minor disturbance. Its color suggests the presence of an older stellar population, likely with moderate star formation. The galaxy’s mass suggests that it is not a dwarf galaxy.
