The galaxy presents an elliptical morphology, appearing elongated with a cigar-shaped structure. The light distribution is relatively smooth, with a centrally concentrated bulge that emits a yellow-orange hue. The outer regions of the galaxy display a gradual fading of light, transitioning from the central yellowish glow to a dimmer, bluer halo. There is no obvious spiral arm structure or prominent dust lanes visible. The overall appearance suggests a relatively evolved stellar population with ongoing, but not excessive, star formation activity. There are no indications of major mergers or significant tidal disturbances in the observed morphology, though some minor disturbances may be present.
