The galaxy presents an overall elliptical morphology, elongated along its major axis, with a smooth, diffuse appearance. A centrally concentrated bulge exhibits a reddish-orange hue, possibly indicative of an older stellar population. The outer regions show a gradual decrease in surface brightness and appear slightly bluer in color, hinting at the presence of younger, hotter stars and ongoing star formation, albeit at a relatively low rate. The galaxy does not display any obvious spiral arm structure or significant dust lanes. There is some suggestion of minor disturbances in the overall shape, possibly indicating a past or ongoing interaction with another galaxy, although no distinct merging companion is visible. The overall shape is elongated, but not to the point of being considered cigar-shaped.
