The galaxy presents as a relatively smooth and featureless object, suggesting an elliptical morphology. The light distribution is concentrated towards the center, indicating a substantial bulge component. The galaxy exhibits a slight elongation with a subtle change in angle with respect to the center. There is a noticeable color gradient, shifting from a yellowish hue in the central region to a redder tone in the outskirts. This could be indicative of an older stellar population dominating the outer regions. Overall, there is no obvious evidence of spiral arms or significant dust lanes. The system appears relatively undisturbed, without major signs of ongoing merging activity.
