The galaxy presents as a relatively compact object with a moderate radial extent. Its morphology appears to be predominantly smooth. The light distribution is somewhat centrally concentrated but lacks a sharply defined core or nucleus. There is a slight asymmetry in the outer regions. The galaxy exhibits a yellowish-white hue, indicating a population of older stars, but with a bluer tint to the disk and other regions of star formation. Based on the slight irregular shape of the disk there may be ongoing or recent interactions. 
