This galaxy appears to be a relatively smooth, elliptical galaxy with an approximate apparent diameter of 3 arcseconds. It exhibits a concentrated central bulge that transitions smoothly into a fainter, more diffuse halo. The color gradient suggests an older stellar population, with the central region appearing more yellow/orange and the outer regions appearing more blue. This could indicate ongoing or recent star formation. There is no clear evidence of spiral arms or a well-defined disk structure. No significant distortions or tidal features are visible.
