This galaxy appears to be a luminous elliptical galaxy, exhibiting a smooth, concentrated morphology. The galaxy's light is dominated by a yellow-orange hue in the center, suggesting an older stellar population. The radial light profile appears centrally concentrated, with a gradual decrease in intensity moving outward. Some irregularities and fainter extended emission suggest the possibility of past or ongoing interactions with other galaxies, or the possibility of a minor disturbance in the morphology. The galaxy is approximately circular in appearance, though there is a slight elongation. The presence of significant yellow light suggests ongoing or recently quenched star formation.
