The galaxy presents as a flattened, elliptical shape. It exhibits a smooth, diffuse light distribution, suggesting a lack of prominent spiral arms or distinct features. The central region appears brighter, indicating a higher concentration of stars and potentially a central supermassive black hole. The color gradient shifts from a yellow-white core to a redder outer halo, which may indicate older stellar populations in the outskirts. There are no obvious signs of ongoing major mergers or tidal disruptions, although there is some subtle asymmetry in the overall shape, possibly hinting at a past minor interaction. Overall, the galaxy appears to be a relatively evolved system with suppressed star formation activity.
