The galaxy presents as a centrally concentrated object with a relatively smooth, diffuse morphology. The central region exhibits a slightly brighter, more compact core. The galaxy appears to be a flattened spheroid, displaying a moderate degree of roundness. Faint, extended features emanate from the central region, indicating a possible disk-like structure, or the remnants of tidal interactions. There are subtle variations in color, with a bluer hue towards the central regions which suggest regions of star formation, while a redder color is present in the periphery which is indicative of older stellar populations. There are signs of mild disturbances or asymmetries in the overall structure. The galaxy shows minimal evidence of major ongoing mergers or significant tidal disruptions. Overall, the galaxy appears to be a relatively quiescent system.
