The galaxy presents as a relatively compact and somewhat elliptical object. Its color profile exhibits a central region that is a very bright white-blue, likely due to concentrated, hot, young stars and potentially an active galactic nucleus. The outer regions show a decreasing light intensity, transitioning to a yellow-red hue, suggestive of an older stellar population with cooler stars. The galaxy appears largely undisturbed, without any prominent tidal features, spiral arm structures, or evidence of a major merger event. There may be slight asymmetrical characteristics in its light distribution. It is observed to have very limited star formation.