The galaxy presents an elliptical morphology with a smooth, diffuse appearance, suggesting it is an early-type galaxy. There's a concentration of light towards the central region of the galaxy, implying a bulge. The color gradient shows a yellow-orange hue at the core, possibly indicating an older stellar population dominated by redder stars. Moving outward, the galaxy's color seems to shift slightly toward green and blue, which could be due to some presence of younger stars or ongoing, albeit subdued, star formation. There's no distinct evidence of spiral arms or prominent dust lanes. Faint disturbances hint at a potential minor interaction or past merger event, but these are subtle. Overall, the galaxy exhibits a relatively undisturbed structure.
