The galaxy presents a generally smooth appearance, with a slightly elongated, cigar-like morphology. It exhibits a dominant central bulge, characterized by a yellowish hue, suggestive of an older stellar population. Fainter, bluish regions are observed extending from the main body. These regions suggest possible ongoing star formation. There is a suggestion of a minor interaction or disturbance in the galaxy's morphology. The overall structure appears relatively undisturbed.
