The galaxy presents as a moderately luminous, early-type galaxy, likely an elliptical or lenticular type. The light is dominated by older stellar populations, inferred from the redder color towards the central bulge. The galaxy displays a smooth and featureless morphology, with no apparent spiral arm structure or dust lanes visible. Its shape appears elongated, deviating from a perfectly circular profile; the axial ratio suggests a cigar-like appearance. There are no signs of a major merger event or significant tidal disturbances, though there may be a minor disturbance. Star formation is low, with a high mass to light ratio. The galaxy exhibits a high degree of central concentration.
