The galaxy presents as a single, relatively smooth object with a concentrated central bulge. The light is dominated by a yellow-orange hue, suggestive of an older stellar population with fewer young, massive stars. There are no prominent spiral arms or distinct features such as dust lanes visible. The galaxy appears nearly spherical. The outer edges fade gradually, indicating a lack of sharp boundaries. There is little, if any, evidence of ongoing mergers or tidal disturbances, and the overall morphology indicates a lack of significant star formation.
