The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. Its shape is elongated, appearing somewhat cigar-shaped rather than perfectly round. The light distribution suggests a fairly homogenous stellar population. There is a clear color gradient, with the central region exhibiting a warmer, yellowish hue, possibly indicating an older stellar population and/or dust content. The outer regions appear bluer, suggesting the presence of some younger stars. Overall, the galaxy appears undisturbed, with no obvious signs of recent major mergers or tidal interactions. The data suggests this galaxy is quite massive, with a moderate amount of star formation occuring.
