The galaxy presents a generally smooth and rounded morphology. It appears to be relatively undisturbed, lacking significant signs of ongoing or recent major mergers, although subtle disturbances or minor interactions cannot be entirely ruled out. The light distribution suggests a centrally concentrated structure with a gradual decrease in luminosity outwards, lacking any prominent spiral arm features or a distinct disk component. The galaxy exhibits a slight color gradient, appearing bluer in the outer regions and subtly redder towards the core, potentially indicative of variations in stellar populations or dust distribution. The galaxy has an estimated size of ~3 kpc and a estimated mass of approximately 10^8 solar masses. Star formation appears to be suppressed.
