The galaxy presents an elliptical morphology, exhibiting a relatively smooth light distribution without prominent spiral arms or a well-defined disk structure. It appears elongated, with a moderate axis ratio, suggesting a deviation from a perfectly spherical shape. The color gradient indicates a central concentration of older stellar populations, appearing more red, with a gradual shift towards bluer hues in the outer regions, potentially indicating the presence of younger stars or ongoing star formation activity in the periphery. Visual assessment indicates a minor interaction or disturbance within the system, as the general shape of the galaxy is somewhat distorted.
