The galaxy presents as an elongated, somewhat cigar-shaped structure. It appears relatively smooth with a concentrated central bulge exhibiting a yellowish hue, indicative of an older stellar population. The outer regions of the galaxy display a bluer tint, suggesting the presence of younger stars and ongoing star formation. There is little evidence of spiral arm structure or significant dust lanes; it may potentially be a lenticular or elliptical galaxy. There is a slight asymmetry to the galaxy, and a faint disturbance is possible in the outer regions, which might indicate a minor interaction. There is no apparent evidence of a major merger event.
