The galaxy presents a generally smooth, elliptical morphology, showing a moderate degree of central concentration. The light distribution appears relatively uniform without prominent spiral arm structures or significant dust lanes. The object exhibits a central bulge that dominates the overall luminosity. The galaxy appears nearly spherical in shape, showing only a slight deviation from perfect roundness. There are no apparent signs of ongoing major mergers or tidal disruptions affecting the galaxy's structure. However, there could be very faint signs of a minor disturbance nearby, possibly indicating a minor merger or interaction. The overall color appears relatively uniform across the galaxy, with a subtle bluer tinge that suggests some ongoing star formation.
