The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The light profile appears relatively uniform, lacking distinct spiral arm structures. There is a color gradient, exhibiting a shift towards redder hues in the central region, which may suggest an older stellar population and less active star formation there, with bluer hues present towards the outside. This implies a possible radial variation in stellar age or dust content. The ellipticity indicates that this object is not perfectly spherical, but appears somewhere in between a perfect circle and a cigar shape. There is no visual evidence of any ongoing major or minor mergers or tidal disturbances.
