The galaxy appears as a smooth, elongated structure with a discernible central bulge. Its overall shape suggests a classification along the lines of an elliptical or lenticular galaxy, exhibiting a cigar-like morphology. The light distribution is concentrated towards the center, with a gradual fading toward the outer edges.

A color gradient is observed, shifting from a yellowish hue in the central region to a bluer tint in the outer parts of the galaxy. This could indicate an older stellar population dominating the core, while younger stars are present in the galaxy's outskirts. There is no prominent dust lane or spiral arm structure visible. There are no clear signs of any major gravitational disturbances or ongoing mergers.
