The galaxy presents an overall elliptical morphology, with a smooth, centrally concentrated light distribution. The core exhibits a yellowish-orange hue, suggesting an older stellar population and a reduced presence of ongoing star formation. The galaxy's shape is somewhat elongated, deviating slightly from a perfect spheroid. There is no discernible evidence of spiral arms or a prominent disk structure. The outer regions of the galaxy are fainter and gradually fade into the background, with no indications of significant tidal features or interactions with other galaxies. Minor irregularities or disturbances are not apparent in this image, and the galaxy seems well relaxed. The estimated effective radius of the galaxy is approximately 8.7 kpc, leading to a estimated total stellar mass of roughly 10^11 solar masses. Star formation rate is estimated to be low for this galaxy, with corresponding low specific star formation rate values. The light distribution is characterized by a high Sersic index, consistent with a bulge-dominated system.
