The galaxy presents as a moderately luminous, early-type system. It exhibits a relatively smooth and regular morphology, with little to no apparent spiral arm structure or significant dust lanes. The overall shape approximates an elliptical form, tending towards a spheroidal appearance. The color gradient suggests a population of older stars dominating its stellar content, likely exhibiting a weak ongoing star formation rate. There is some marginal evidence of a possible minor disturbance, but does not appear to be undergoing a major merger.