The galaxy presents a generally smooth, elliptical morphology. A concentrated central bulge is observed, surrounded by a fainter, more diffuse halo of stellar light. The color gradient suggests an older stellar population, with a yellowish-red hue dominating the central region. There are hints of a faint, flattened disk structure surrounding the bulge, potentially indicating the presence of a spiral arm, however it is barely noticeable. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There is some very minor disturbance in the light surrounding the galaxy that may indicate it is merging with a very small object, but it is likely to be a result of noise in the image.
