The galaxy appears as a luminous, centrally concentrated object with a somewhat elliptical morphology. The light profile appears smooth and diffuse, lacking any distinct spiral arm structures or prominent dust lanes. The galaxy exhibits a central bulge, although it is not particularly pronounced, and the overall light distribution is relatively uniform. A subtle color gradient can be observed; the central region appears slightly redder, potentially indicating an older stellar population, whereas the outer regions seem bluer, suggesting the presence of younger, hotter stars. There is also a minor indication of a slight warp or irregularity in its structure, which could potentially point to a past merger event or tidal interaction. The object presents a morphology consistent with an early-type or lenticular galaxy, lacking the characteristics of a late-type spiral.
