The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There's a notable lack of distinct spiral arms or well-defined features indicative of active star formation. The color profile suggests an older stellar population, with a dominant reddish-yellow hue, particularly pronounced in the central region. This color gradient implies a decreasing presence of younger, bluer stars towards the core. The galaxy appears largely undisturbed, with no obvious signs of major mergers or tidal interactions. Minor disturbances cannot be ruled out. It exhibits a high degree of roundness and appears to be relatively isolated within its immediate field, lacking any close companion galaxies that might influence its morphology or evolution.
