The galaxy presents an overall smooth appearance, suggesting an elliptical morphology or a spiral galaxy seen at a high inclination. The central region exhibits a concentrated, bright core, indicating a potentially high stellar density or an active galactic nucleus. The light distribution falls off gradually from the center, exhibiting a somewhat elongated shape, possibly classified as a cigar shape. The galaxy's color is primarily yellowish-orange, suggesting an older stellar population with a reduced rate of current star formation. There appears to be little to no evidence of spiral arms or dust lanes, reinforcing the smooth, elliptical-like characteristics. No signs of major mergers or tidal disturbances are readily apparent, although a subtle asymmetry might hint at a minor interaction or past merger event.
