The galaxy presents a smooth, elliptical morphology. It appears to be largely featureless, lacking defined spiral arms or a prominent central bar. The light distribution is concentrated towards the core, with a gradual decrease in intensity towards the outer edges. The galaxy exhibits a slightly elongated shape. Color gradients are subtle, with a central region showing a yellowish hue, possibly indicative of an older stellar population, transitioning to slightly bluer tones in the outer regions, suggestive of ongoing star formation. There is no obvious evidence of a major merger or significant tidal disturbances.
