The galaxy presents as a centrally concentrated object with a generally smooth morphology. It appears to be elliptical in shape, though it is relatively round. The central region is bright and yellowish-white, indicating a high density of older stars. Fainter blue-ish emissions are visible towards the one side, hinting at the presence of younger stellar populations and ongoing star formation. There's a suggestion of minor morphological disturbance. The galaxy does not appear to be undergoing any major merging events. 
