The galaxy presents as a relatively smooth, elliptical morphology. Its color profile suggests an older stellar population, with a dominant yellowish-red hue. The galaxy appears somewhat compact with no visible spiral arm structures or distinct dust lanes. The shape is somewhere between round and cigar shaped. There is no strong evidence of ongoing major merger activity, though the possibility of a minor interaction cannot be excluded due to some slight asymmetry. The overall smooth appearance indicates a relatively quiescent state of star formation.
