The galaxy presents as a lenticular or early-type spiral with a notably smooth morphology and an elliptical shape. It exhibits a central bulge region that dominates the overall luminosity profile, with a gradual decrease in brightness towards the outer regions. The color gradient suggests a population of older stars throughout the galaxy, with a slightly bluer hue in the disk possibly indicating the presence of some younger stars and ongoing, although likely subdued, star formation. Evidence of spiral arms or distinct features within the disk is minimal, suggesting a relatively undisturbed and evolved system. The isophotes appear largely regular, with no obvious signs of major mergers or significant tidal disturbances. The object does not appear highly inclined.
