The galaxy presents as a relatively smooth, elliptical structure, with an apparent lack of distinct spiral arms or significant features. The light is concentrated toward the center, indicating a prominent bulge. The morphology appears to be tending more towards an elliptical shape rather than a disk-like structure. There is no apparent major merger or significant tidal disturbance readily visible in the immediate vicinity, although some minor asymmetry or disturbance is present. It has an overall color leaning towards a redder hue, suggesting a population of older stars. The star formation activity is low.
