The galaxy appears as a smooth, elliptical structure, elongated in shape, with a cigar-shaped morphology. The object exhibits a concentrated central bulge, with a gradual decrease in luminosity extending outwards. Its color profile shows a redder hue, indicating an older stellar population and a potentially lower rate of star formation. No spiral arms or distinct disk features are visible. There are no obvious signs of recent major merger activity or significant tidal disturbances; however, a subtle asymmetry suggests possible minor past interactions. The galaxy's overall smoothness points towards it being a relatively evolved system.
