The galaxy appears to be a relatively smooth, elliptical type, or possibly a lenticular galaxy viewed nearly face-on. It presents a centrally concentrated light profile, with the majority of its luminosity focused towards the core. A prominent bulge is discernible, exhibiting a yellowish-orange hue, suggestive of an older stellar population. This feature implies a lack of significant recent star formation within this region. Extending outward from the bulge, a fainter, bluer halo is observed, which could indicate the presence of a small disk or extended envelope of younger stars. The overall morphology appears undisturbed, lacking any obvious signs of recent or ongoing major mergers. However, the irregular edges suggest the possible on-going process of a minor merger. The galaxy shows no pronounced spiral arm structure or prominent dust lanes. The light distribution exhibits a fairly symmetrical pattern, suggesting that it is likely a regular elliptical galaxy that has reached a stable equilibrium configuration.
