The galaxy presents as a relatively smooth, round structure, indicative of an elliptical morphology. The light distribution suggests a concentrated central bulge that gradually fades outwards, characteristic of an older stellar population. The central region exhibits a yellowish hue, which likely indicates a higher concentration of older, redder stars. Progressing outwards, the galaxy's periphery displays a slightly more blue-green tint, possibly from younger, hotter stars. There's no strong evidence of spiral arms or a pronounced disk. The galaxy appears mostly undisturbed, with only minor potential indications of tidal effects.
