The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. There is little evidence of spiral arms or significant disk features. The light distribution is centrally concentrated, with a gradual decline in intensity towards the outer edges. The galaxy exhibits a yellow-red hue, indicating a population of older stars. No evidence of recent major merging events or significant tidal disturbances is readily apparent, though minor disturbances cannot be ruled out due to the image resolution. Overall, the galaxy appears as a mature system with limited ongoing star formation.
