The galaxy presents a generally smooth, elliptical morphology, with a bright, concentrated central bulge that gradually diffuses into the outer regions. The color profile suggests a population of older stars, based on the redder hues present, particularly towards the central regions. However, some blue regions indicate the presence of a young star population. No distinct spiral arm structure or prominent dust lanes are readily apparent. There is no clear evidence of a major ongoing merger event, although there may be subtle asymmetries or minor disturbances in the outer halo, possibly indicative of past interactions or minor mergers. The roundness of the galaxy suggests it is most likely an elliptical galaxy type. Overall, the galaxy appears to be relatively evolved, potentially in a transitional phase between actively star-forming spiral or irregular galaxies and quiescent elliptical galaxies.
