The galaxy presents a mostly smooth, elliptical morphology. Its overall shape is somewhat irregular, exhibiting a slight elongation, but it lacks well-defined spiral arms or a distinct disk structure. The central region of the galaxy appears as a bright, concentrated core, suggestive of a substantial galactic nucleus. There is some disturbance of the galaxy structure, hinting at tidal interactions or the remnants of a past merger event. The observed color gradient is suggestive of an aging stellar population. The galaxy's estimated size indicates it is a moderately sized system. The estimated mass, derived from photometric redshift data, positions this galaxy within the typical range for galaxies of this type. The moderate star formation rate indicates it is not intensely star-forming, but still shows some activity.
