The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a dominant central bulge that appears yellowish-white, suggesting a population of older stars. Surrounding the bulge is a fainter, bluish halo. The galaxy does not display prominent spiral arms or a well-defined disk. Its overall shape is elongated, somewhere between round and cigar-shaped, with a slight deviation from a perfect ellipse, though it is difficult to determine if it is truly disturbed. There appears to be ongoing star formation, albeit at a moderate level, as indicated by the subtle blue tint in the outer regions. There is no evidence of a major merger event, though possible minor disturbances can't be ruled out entirely.
