The galaxy appears to be an elliptical type, characterized by a smooth, centrally concentrated light distribution. The color gradient suggests a redder core, possibly indicating an older stellar population dominating the central region. A gradual bluing trend towards the outer edges may indicate the presence of some younger, bluer stars in the galaxy's periphery, though the overall color profile suggests minimal ongoing star formation. The galaxy has a fairly regular, somewhat elongated shape with no obvious signs of spiral arms or a distinct disk component. There is no visual evidence of any major tidal disturbances or recent merger events affecting its structure, although there is slight asymmetry in its outer light distribution.
