The galaxy appears as a relatively compact, elliptical-like structure. It exhibits a smooth, diffuse light distribution with a slightly elongated morphology. The central region is brighter, suggesting a concentration of stars towards the core. There is little evidence of prominent spiral arms or distinct features. A subtle color gradient is visible, with the core exhibiting a yellower hue, potentially indicating an older stellar population, while the outer regions have a bluer tint, possibly suggesting a younger population or ongoing star formation. There is a faint, bluish feature that might indicate the presence of a small disk. Overall, the galaxy appears relatively undisturbed, with no signs of major ongoing mergers or tidal interactions.
