The galaxy presents as a single, relatively smooth object. It exhibits a concentrated, rounded morphology with minimal discernible substructure. The color is a gradient, shifting from a slightly bluer hue in the center to a redder periphery, though overall the galaxy presents as primarily redder. There is no apparent spiral structure, nor any obvious signs of tidal disruption or active galactic nuclei-related jets. The light distribution falls off smoothly from the center without any prominent bright or dark patches. It appears that the galaxy may be in a relatively late stage of its evolution, as implied by the dominant redder color, consistent with an older stellar population.
