The galaxy presents as a somewhat elongated, diffuse object with a concentrated central bulge. It exhibits a smooth morphology, lacking the well-defined spiral arms typically associated with late-type galaxies. There is a slight color gradient, with the central bulge appearing more yellow/orange, possibly indicating an older stellar population. The outer regions exhibit a bluer tint, hinting at the presence of younger, hotter stars. The overall form suggests an elliptical or lenticular galaxy type, though higher resolution imaging would be required to confirm this. There is no clear evidence of significant star formation, though a faint hint of blue in the surrounding regions indicates the presence of some young stars. No major tidal disturbances or signs of recent mergers are apparent. The galaxy appears relatively isolated and undisturbed.
