The galaxy presents an elliptical morphology, with a smooth, diffuse light distribution. There is a lack of distinct spiral arms or a central bar structure. The galaxy exhibits a color gradient, transitioning from a slightly bluer hue in the central region to a redder tone in the outer regions. The overall color suggests an older stellar population. There is no evidence of any ongoing major merger activity or significant tidal disturbances affecting its structure. The galaxy appears relatively isolated and undisturbed within the observed field.
