The galaxy appears as a centrally concentrated, elliptical-like structure. It presents with a smooth, mostly featureless morphology, lacking defined spiral arms or a prominent disk. The central region exhibits a bright, concentrated luminosity, suggesting a significant concentration of older stars or potentially an active galactic nucleus. The galaxy displays a yellowish-red hue, which indicates a stellar population dominated by older, redder stars, consistent with a lower rate of star formation. The overall shape is somewhere between round and elongated, appearing somewhat cigar-shaped. There's no obvious evidence of major tidal disturbances or ongoing mergers in this image.
