The galaxy presents as a lenticular or edge-on spiral galaxy. There is a central bulge that appears smooth and concentrated. The disk is elongated and slightly inclined relative to our line of sight, giving it a cigar-shaped appearance. The disk's light distribution seems relatively uniform, lacking prominent spiral arm structures and only hints of dark dust lanes on the sides closest to us. The galaxy exhibits a moderately red color, suggesting a population of older stars with lower star formation. There is no visible evidence of a significant ongoing merger or tidal disturbance, although subtle asymmetries might indicate past interactions or minor disturbances. The overall morphology suggests a galaxy with a large stellar mass and a relatively low star formation rate.
