The galaxy presents as a moderately sized, relatively luminous object with an apparent slightly elliptical morphology. The core region is bright and concentrated, suggesting a significant stellar density. The galaxy displays a relatively smooth overall appearance, with only subtle indications of internal structure or distinct spiral arms. The galaxy exhibits a color gradient, appearing bluer toward the outer regions and redder toward the core, potentially indicating ongoing star formation in the outskirts and an older stellar population in the central bulge. There are hints of faint, disturbed features extending outward from the main body of the galaxy, suggestive of a possible past interaction or merger event.
