The galaxy presents a roughly elliptical morphology, suggesting a classification towards the lenticular or early-type spiral category. The galaxy exhibits a central bulge that appears relatively bright and well-defined, surrounded by a fainter, more diffuse disk component. Within the disk, there is subtle evidence of spiral arm structure, although the arms are not sharply defined. The overall color profile indicates a dominant population of older stars, likely resulting in the reddish tones observed. The galaxy is seen at a moderate inclination angle. There appear to be no major mergers or tidal disturbances. There does not appear to be a great deal of star formation occurring. Overall, the galaxy presents characteristics typical of evolved galaxies in the local universe.
