The galaxy presents as a somewhat elliptical, disk-like structure with a prominent central bulge. The luminosity appears concentrated towards the core, with a gradual decrease in intensity towards the outer edges. The disk exhibits subtle features, possibly indicative of spiral arm structures, though these are not sharply defined. The overall color profile suggests a mix of stellar populations, with a relatively redder hue in the central bulge potentially indicating older stars and a bluer tint in the disk hinting at ongoing star formation. There may be signs of minor gravitational interactions, though no significant merger activity is immediately apparent. The shape is predominantly round, verging slightly towards an elongated form.
