The galaxy presents a primarily elliptical morphology, with a smooth, concentrated light profile. The central region exhibits a bright, yellowish core, suggesting a population of older stars. Proceeding outward, the light gradually fades into the surrounding halo. There is an absence of well-defined spiral arms or prominent dust lanes. The overall shape appears slightly elongated, trending toward an "in-between" form, rather than perfectly circular or cigar-shaped. There is a possible minor perturbation or asymmetry in the galaxy's outer regions. No clear evidence of a major ongoing merger is apparent, but a small disturbance cannot be ruled out. The galaxy's color indices suggest moderate star formation is occurring, but may also be influenced by older stellar populations.
