The galaxy presents as a relatively compact object with a smooth, elliptical morphology. There is no discernible spiral structure. The galaxy appears to be undergoing a merger, presenting dual nuclei. The color of the light emitted suggests a population dominated by older stars, although the presence of redder hues in the more diffuse region indicates some ongoing, although likely subdued, star formation activity. The overall round appearance suggests that it's not highly inclined with respect to our line of sight. There are no clear tidal tails.
