The galaxy presents as a single, fairly smooth object, roughly elliptical in shape. The core region appears significantly brighter and exhibits a yellow-orange hue, suggesting a population of older stars. A slightly greenish tint is visible in the outer regions of the galaxy, potentially indicating the presence of younger stellar populations or ionized gas, although the overall star formation rate appears to be relatively low. There are no obvious spiral arms or bar structures. The light distribution appears relatively uniform, indicating no signs of major mergers or significant tidal disturbances. The apparent elongation indicates that it is not a perfect sphere. 
