The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal in shape with no discernible spiral arm structure. The light distribution shows a concentration towards the center, indicating a substantial galactic bulge. Coloration is generally consistent, displaying a yellow-orange hue, suggesting a stellar population dominated by older, less massive stars, and relatively low levels of ongoing star formation. The galaxy does not appear to be undergoing any major mergers or significant tidal disturbances. There is no evidence of dust lanes or prominent gas features in the image. The isophotes appear fairly regular with no obvious boxiness or diskiness. The overall impression is that of a relatively evolved and undisturbed elliptical galaxy.
