The galaxy presents as a largely elliptical structure with a smooth, diffused appearance. Its core region exhibits a bright yellowish hue, suggesting an older stellar population. A subtle gradient of color is observed moving outwards from the core, transitioning to a bluer tone in the outer regions, potentially indicative of more recent, albeit limited, star formation activity. No distinct spiral arms or bar structures are discernible. The overall shape is somewhat elongated, though tending toward a more rounded profile. There is no obvious evidence of ongoing major mergers or strong tidal disturbances affecting the galaxy’s morphology. The galaxy appears relatively isolated, showing no strong interactions with nearby galaxies. The color profile suggests a potential transition galaxy, perhaps between a quiescent elliptical and a more actively star-forming system.
