The galaxy presents as an elongated, cigar-shaped structure. The central bulge exhibits a yellowish-white hue, indicating a population of older stars. The disk is not well-resolved, appearing somewhat amorphous and lacking distinct spiral arm structure. A smooth, rather than clumpy texture suggests a relatively quiescent star formation rate. Faint extensions of diffuse light appear to extend outwards from the main body of the galaxy, although these are not sharply defined. No evidence of major merger events or significant tidal disturbances are apparent from its morphology. Overall, the galaxy gives the impression of a relatively evolved system.
