This galaxy appears to be an elliptical galaxy with a smooth, diffuse morphology. The light is concentrated towards the center, which is the brightest region, and gradually fades outwards. It exhibits a spheroidal shape, appearing largely circular in this projection. There is no apparent evidence of spiral arms or a prominent disk. The galaxy does not show any signs of significant ongoing mergers or major disturbances, though there might be some minor irregularities in the outer regions, this could be due to noise. The color profile suggests a population of older stars, contributing to the redder hue of the galaxy in the observed bands. The rate of star formation is likely low. 
