The galaxy appears to be an elliptical morphology. Its light profile is smooth and centrally concentrated, with a gradual decrease in luminosity outwards from the core. The galaxy exhibits a generally featureless appearance, lacking spiral arms or prominent dust lanes. The color is consistent with an older stellar population, with the central region appearing slightly yellower than the outer regions. No obvious signs of ongoing major merger activity or significant tidal disturbances are apparent. The galaxy presents a somewhat oblate shape, deviating slightly from a perfect sphere. Overall, the observed features point towards a galaxy dominated by an older stellar population with minimal star formation.
