This galaxy exhibits a roughly elliptical morphology, although some irregularities are present in its overall shape. The central region displays a concentrated, bright core that appears primarily blue in color, suggesting the presence of a population of hot, young stars and potentially active star formation. The outer regions transition into a more diffuse and less distinct halo, showing a gradual fading in brightness and a slight shift towards redder hues, which could indicate an older stellar population. There is evidence of minor disturbances or asymmetries in the galaxy's structure, potentially indicating past or ongoing gravitational interactions or minor merger events. Faint, extended features may be present, but they are difficult to resolve due to image quality.
