The galaxy appears to be an elliptical galaxy, characterized by a smooth, relatively featureless morphology. It exhibits a concentrated central bulge that gradually fades into the outer regions. The galaxy shows a nearly round shape. There are no clear signs of spiral arms or a prominent disk structure. The color profile suggests a population of older stars, with a yellow to reddish hue dominating the central region. Some bluer patches are present within the galaxy, indicative of younger stellar populations and ongoing, but slow, star formation activity. There is no evidence of a major ongoing merger or significant tidal disturbances. The overall impression is that of a relatively relaxed and evolved system.
