The galaxy appears to be a relatively bright, elliptical galaxy at a considerable distance. Its morphology indicates it is largely smooth and rounded, lacking distinct spiral arms or a prominent disk structure. The galaxy exhibits a concentrated central bulge that radiates significant light, implying a dense population of stars in the core. The color profile suggests a population dominated by older, redder stars. There is little evidence of ongoing star formation. Its overall structure appears undisturbed, with no readily apparent signs of major mergers or tidal distortions. The galaxy is compact and appears to have a high mass.
