The galaxy presents a generally smooth, elliptical morphology. There is little evidence of spiral arm structure or a prominent disk. The overall shape is moderately elongated, leaning towards an in-between shape rather than perfectly circular or cigar-shaped. The color appears to be a somewhat muted cyan, indicative of either intermediate-age stars or high red-shift. There is no obvious nucleus or central bulge discernible within the observed resolution. Additionally, there are hints of a minor disturbance in the outer halo of the galaxy, such as a slight irregularity in its overall shape or a faint tidal feature that could be the result of a past interaction. No major merger events or strong tidal distortions are immediately apparent.
