The galaxy appears as a moderately bright, centrally concentrated object. Its overall morphology seems relatively smooth and elliptical, displaying a high degree of circular symmetry. There is little discernible internal structure such as spiral arms or dust lanes visible in this image. The light distribution suggests a single bulge component dominating the light profile. Given the observed color indices, the galaxy exhibits a redder color, suggesting a stellar population dominated by older, lower-mass stars. Star formation activity appears to be relatively low. There is no obvious evidence of tidal features or morphological disturbances indicating recent major merger events, however, minor interactions cannot be ruled out. The apparent size of the galaxy is small, hinting at a compact structure.
