The galaxy presents as a largely smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, appearing somewhat more akin to an oval than a perfect circle. The luminosity profile suggests a gradual decrease in brightness from the core outwards. The central region is dominated by a yellowish glow, possibly indicative of an older stellar population. Moving outwards, the galaxy transitions into a bluer halo, which could be associated with younger stars or a population with higher metallicity. There are no obvious spiral arm structures or signs of significant dust lanes. Minor disturbances cannot be ruled out, but there's no prominent evidence of a major ongoing merger event or tidal disruption. The overall impression is that of a relatively evolved system.
