This galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that appears bright and somewhat spherical. The surrounding halo fades gradually from the core, indicating a diffuse stellar population. There is a subtle elongation present, transitioning from a round shape to a somewhat cigar shape, suggesting it's not perfectly spherical, but more of a slightly flattened spheroid. No distinct spiral arm structures are discernible in the image, and the galaxy exhibits a general lack of significant features or disturbances, pointing towards a relatively quiescent state with a low star formation rate. The colour profile seems to show a yellow-white hue, pointing to an older stellar population. There is no apparent evidence of any significant merger activity.
