The galaxy appears to be an elliptical type, exhibiting a generally smooth, diffuse light distribution. It has a slight elongation, suggesting a shape somewhere between perfectly round and cigar-shaped. The central region of the galaxy displays a higher concentration of light, transitioning gradually to a fainter halo. There is a subtle color gradient, with the core appearing slightly yellower than the outer regions, which are more bluish. This might indicate older stellar populations in the core, and the possible presence of more recent star formation, as evidenced by the galaxy's moderate star formation rate, especially in the outer disk. There are no clear signs of spiral arms or significant dust lanes. Based on the merging fraction estimates, the galaxy shows no significant signs of any merger events, only some minor disturbances.
