The galaxy presents a smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct bar structure. The galaxy exhibits a concentrated central bulge that fades gradually into an extended halo. The color profile is generally redder, suggesting a population of older stars and a relatively low rate of current star formation. The galaxy is nearly circular in appearance. There is no evidence of significant tidal disturbances or ongoing mergers, suggesting it is a relatively isolated system.
