The galaxy appears to be an elliptical type. It exhibits a smooth, centrally concentrated luminosity profile with a gradual decrease in brightness moving outward from the core. The galaxy displays a flattened, cigar-like shape. There is no apparent dust lane, spiral arm structure, or other signs of significant recent merger activity or disk-like features. The core region shows a bright, concentrated emission, possibly indicating an active galactic nucleus. The galaxy's color is generally redder, suggesting an older stellar population, with a slight bluer hue toward the central region. The galaxy does not appear to have any major disturbances in its morphology.
