The galaxy presents a largely featureless, smooth morphology, exhibiting characteristics consistent with an elliptical galaxy. It appears nearly round in projection, with a concentrated central bulge that gradually fades into the outer regions of the galaxy. The color gradient suggests a population of older stars, particularly in the central region, with a slightly bluer hue as the light extends outwards. There is no clear evidence of spiral arms, a prominent disk structure, or any significant tidal disturbances or ongoing merger events. Overall, the galaxy appears relatively isolated and undisturbed, presenting a regular, symmetrical structure.
