The galaxy presents a relatively smooth and rounded morphology, suggesting an elliptical or lenticular classification. There is a subtle elongation, deviating slightly from a perfectly circular shape. The central region exhibits a bright, concentrated core, indicative of a significant concentration of stars. The galaxy appears to be in a relatively isolated environment, with no clear signs of ongoing major mergers. However, subtle asymmetries or minor disturbances in the outer regions suggest the possibility of past interactions or minor accretion events. Overall, this galaxy appears to be a fairly evolved and quiescent system.