The galaxy appears to be a relatively smooth, elliptical-like system. It exhibits a concentrated, bright central bulge that gradually fades into a diffuse outer halo. There is little visible evidence of distinct spiral arms or significant dust lanes. The color gradient suggests a population of older stars, with the central regions appearing more yellow/reddish, indicating a higher concentration of evolved stars. While the overall form is smooth, there may be a faint, disturbed feature or tidal tail on the left side, suggesting a potential past interaction with another galaxy.
