The galaxy presents as an elliptical structure with a smooth, diffuse morphology. It exhibits a concentrated central bulge that appears to be spheroidal in shape, dominating the overall luminosity. The color gradient transitions smoothly from a yellowish core to a slightly redder outer halo, suggesting a dominant population of older stars. There is a subtle hint of a minor disturbance in the upper left corner of the galaxy. The galaxy lacks any discernible spiral arms or prominent dust lanes, consistent with a classification of elliptical. The shape is roughly round. No obvious tidal tails or other signs of a recent major merger are apparent.
