The galaxy presents a somewhat elliptical morphology. The light distribution appears relatively smooth, with a central, brighter region indicative of a galactic nucleus. There is no apparent spiral arm structure, and its disk fraction is relatively small. The galaxy shows a slight deviation from perfect roundness; it is more in between round and cigar-shaped. There is a hint of a possible tidal feature or minor disturbance on one edge, but this is not conclusive. The object appears quiescent in terms of star formation, and there is a relatively low amount of star formation throughout. It doesn't seem to be undergoing a major merging event. The color index of the object indicates that it is mostly composed of old stars with very little dust.
