The galaxy presents a generally smooth, elliptical morphology, lacking defined spiral arms or a prominent disk structure. It appears largely featureless, with a concentrated central bulge that dominates the overall light profile. The galaxy exhibits a relatively round shape. There is no strong visual indication of ongoing major mergers or significant tidal disturbances, however minor disturbances may be present. Based on its color, the galaxy is composed primarily of older stars and has a low rate of star formation.
