The galaxy appears to be an elliptical galaxy, exhibiting a smooth, spheroidal morphology with no discernible spiral arms or distinct disk structure. It possesses a concentrated central bulge that dominates the overall luminosity profile. The galaxy presents a yellowish-orange hue, suggestive of an older stellar population with a lower rate of ongoing star formation. There is a lack of blue color indicative of young, hot stars. The object appears to be relatively isolated, with no signs of major tidal disturbances or ongoing mergers, although some minor interaction might be possible. Its overall round shape indicates a relatively dynamically relaxed system. The estimated size places this galaxy among larger galaxies.
