The galaxy presents as a relatively smooth structure with a somewhat disturbed morphology. There is a central, bright bulge region exhibiting a yellowish-orange hue, suggestive of an older stellar population. The overall shape of the galaxy is somewhat elongated, tending towards a cigar shape. There is an indication of a possible minor disturbance, potentially a small companion or interaction, as evidenced by the slightly asymmetric structure. The general color indicates a moderate degree of star formation.
