The galaxy presents a generally smooth morphology with a slight elongation. It exhibits a concentrated central bulge that is primarily yellow, suggesting an older stellar population with a lower rate of star formation. Fainter, more diffuse regions extend outwards from the central bulge. There appears to be a very weak disk-like structure, although no spiral arms or bar features are visible. The overall color profile suggests a transition from older stars in the center to somewhat younger stars in the outer regions. There is no indication of any ongoing major merger activity or significant tidal disturbances. The galaxy appears to be relatively isolated in its environment, without any obvious signs of interaction with nearby galaxies.
