The galaxy presents a morphology suggestive of a late-stage spiral or an early elliptical galaxy. The overall shape is oblong, appearing somewhat cigar-shaped, with a noticeable central bulge that dominates the visual appearance. This bulge exhibits a yellowish-orange hue, potentially indicative of an older stellar population. Faint, diffuse disk-like structures extend from the bulge. These arms display subtle color gradients, with regions of bluer tones suggestive of ongoing star formation activity, albeit at a relatively low rate. The overall smoothness of the galaxy suggests a degree of morphological maturity, lacking prominent spiral arm structures or significant dust lanes. Evident asymmetries are minimal, with no clear indication of a major merger event, though subtle disturbances cannot be ruled out.
