The galaxy appears to be a relatively smooth elliptical or lenticular galaxy, exhibiting a concentrated central bulge. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy's overall shape is close to round, with a slight deviation suggesting a subtle ellipticity. Color gradients suggest a population of older stars dominating the stellar composition. The galaxy is mostly smooth, with only minor evidence suggesting a possible past interaction or minor disturbance but it is mostly undisturbed. The object has a moderate rate of star formation.