The galaxy presents a generally smooth and rounded appearance. It lacks a pronounced disk or spiral arm structure and does not appear to be undergoing any major merging activity, though minor disturbances cannot be entirely ruled out given the image quality. The galaxy exhibits a concentrated central region, which likely represents a galactic bulge. The color profile suggests a population of older stars. Star formation rates are likely low, and the object is relatively massive. The estimated size places this galaxy in the realm of average for galaxies at its redshift.
