The galaxy presents as a relatively smooth, elliptical-like structure. It is elongated, with the major axis appearing to be approximately twice the length of the minor axis. The central region exhibits a high concentration of light, indicative of a prominent bulge. The color appears to be primarily yellow-orange, suggesting a stellar population dominated by older, redder stars. There is a gradual decrease in light intensity from the center outwards, with no distinct spiral arm features or dust lanes visible. The galaxy appears to be relatively undisturbed, with no obvious signs of ongoing mergers or tidal interactions.
