The galaxy appears as a centrally concentrated, relatively smooth structure with an elliptical morphology. It exhibits a yellowish hue, indicating a population of older stars. There's a slight elongation, but overall the shape is close to circular. No distinct spiral arms or prominent dust lanes are visible. There is some subtle indication of a minor disturbance in the structure, possibly hinting at a past or ongoing interaction. The galaxy is likely quite massive and exhibits a low to moderate rate of star formation.
