The galaxy appears as a somewhat smooth, luminous object with a generally round morphology. The central region exhibits a brighter, concentrated luminosity, suggesting a possible bulge or core. A fainter extension of light is observed adjacent to the bright center region, potentially representing a disk or tidal feature. There is an amorphous structure nearby that could possibly be a tidal feature or another smaller galaxy. The galaxy appears to be relatively isolated, with no obvious signs of ongoing major mergers or significant tidal distortions beyond the possible feature that is a disk or tidal feature. Based on the red color, a evolved stellar population with moderate star formation activity is likely to be present.
