The galaxy appears to be a relatively smooth elliptical galaxy, exhibiting a concentrated central bulge that gradually fades into a less defined halo. It presents a soft, diffuse glow. There is little evidence of spiral arm structure or significant dust lanes. The object's color profile shows a generally blue-ish hue, suggesting a population of relatively young, hot stars, or recent star formation, especially toward its outer edges. There may be a very slight extension or distortion, hinting at a potential past interaction, but this is not conclusive from the image alone. The object is largely undisturbed, exhibiting high symmetry. The light distribution suggests the possibility of a bulge-dominated system.
