The galaxy appears to be an elliptical type. The morphology exhibits a smooth, centrally concentrated light distribution. The isophotes are generally rounded, lacking any obvious strong disk or spiral arm features. There is a slight elongation, but overall the shape is close to circular. The color profile suggests an older stellar population, with a yellowish-red hue dominating the central region. The outer regions appear somewhat bluer, which could indicate some ongoing, but minimal, star formation in the outer parts of the galaxy. There's no visual evidence of any major merger events or significant tidal disturbances affecting the structure. Any irregularities appear to be minor. Overall, the galaxy appears relatively undisturbed.
