The galaxy presents an elliptical morphology. It exhibits a smooth light distribution, lacking any obvious spiral arm structures or prominent dust lanes. The central region displays a concentrated luminosity, suggesting a dense stellar population or a possible active galactic nucleus. The color gradient transitions from a yellowish-white core to a redder halo, indicative of older stellar populations in the outer regions and a higher concentration of younger, bluer stars in the central region. The shape appears largely symmetrical, with no indications of significant tidal interactions or major mergers, however some minor disturbances cannot be ruled out. Overall, the galaxy appears to be a relatively evolved system. The estimated size based on half light radius, suggests it is a moderate-sized galaxy.
