The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The light profile suggests a dominant bulge component, exhibiting a yellowish-orange hue. The object displays a high degree of central concentration. There is no evidence of spiral arm structure or significant dust lanes. Faint, extended light may be present along the major axis, but this could be due to image artifacts. There are no obvious signs of ongoing mergers or tidal disturbances, although some faint light could be evidence of minor disturbances. The shape of the ellipse is closer to "in between" than distinctly round or cigar-shaped. Overall, it is a relatively undisturbed galaxy with low star formation.
