The galaxy presents a mostly smooth, elliptical morphology with a high degree of central concentration. The core region displays a brighter, yellowish-white hue, suggesting an older stellar population. Moving outward from the core, the galaxy fades into a less distinct disk with a bluish tint to the inner parts of the disk. There are no obvious spiral arm structures, though some subtle irregularities are present suggesting minor disturbances to the galaxy's structure. The galaxy has a somewhat cigar shape, with the longest dimension estimated to be around 6 kpc. The general appearance suggests the galaxy is currently not undergoing any major mergers, though possible minor interactions in its past could have contributed to the observed features.
