The galaxy presents a generally smooth morphology with a central concentration of light. The core region displays a bright, yellowish hue, suggesting an older stellar population. The overall shape of the galaxy is somewhere between round and elliptical, with only very slight elongation. There is some subtle evidence of a disk or spiral structure. The galaxy shows no signs of major mergers or significant tidal disturbances, such as prominent tails or asymmetrical features, though minor disturbances are possible. Based on the color gradients, the galaxy likely has very low ongoing star formation. The estimated size suggests a moderately large galaxy.
