The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a slightly elliptical morphology, appearing mostly round in shape. There is no clear evidence of spiral arms or a prominent disk structure. The color gradient suggests an older stellar population, with a redder hue in the central region, which could indicate a concentration of evolved stars or dust. Faint, bluer regions exist towards the outer edges. There is minimal evidence of significant tidal disturbances or ongoing major merger activity, with perhaps a hint of a minor disturbance in the overall structure. Overall, this galaxy appears to be a relatively quiescent, evolved system.
