The galaxy presents as a largely featureless spheroid. The light is concentrated at the center, forming a bright, diffuse core. The galaxy exhibits a radial decrease in luminosity from its core outwards. The shape is approximately round, with no clear evidence of spiral arms or a prominent disk structure. There's little to no visible indication of ongoing mergers or major disturbances in its structure. The color appears to be mostly consistent across the galaxy, with a slight tendency towards redder hues in the center, suggesting an older stellar population. Star formation appears to be minimal, if any, based on the uniform color and lack of blue regions associated with younger, hotter stars. The outskirts of the galaxy gradually fade into the background sky, suggesting a smooth density profile.
