The galaxy presents as a moderately luminous, early-type system. It exhibits a smooth, centrally concentrated morphology, with little discernible disk structure or spiral arm features. The overall shape is more in-between round and cigar shaped. The color profile suggests a relatively evolved stellar population, with a redder hue dominating. There is no obvious sign of recent major merger activity or significant tidal disturbances affecting its structure. Star formation rate is considered to be low. The galaxy appears generally isolated in its local environment, with no immediately apparent companions or signs of interaction.
