The galaxy presents as a moderately bright, elliptical object with a smooth, diffuse light distribution. Its shape is elongated, appearing cigar-shaped, with the major axis significantly longer than the minor axis. The central region exhibits a concentrated luminosity profile, indicating a possible bulge component. The color appears yellowish, suggesting an older stellar population with a low rate of ongoing star formation. There is no visible evidence of spiral arms or dust lanes. No signs of major mergers or tidal disturbances are apparent.
