The galaxy presents as a moderately bright, elliptical-like structure, exhibiting a smooth and concentrated morphology. It displays a yellowish-orange hue, suggestive of an older stellar population. There is a slight elongation, with a ratio of the major to minor axis suggesting it is not perfectly spherical but rather somewhat cigar-shaped. The light is centrally concentrated. There is no presence of defined spiral arms or prominent dust lanes. The morphology suggests that it has likely undergone significant evolutionary processes, possibly including past mergers, resulting in the observed smooth light distribution. There is no obvious sign of ongoing major mergers or significant tidal disturbances. The estimated size is about 8 kpc in radius. The mass is quite large at around 10^11 solar masses. The star formation rate is likely to be low.
