The galaxy presents a generally smooth and rounded morphology. The light distribution appears relatively even across its extent, suggesting a lack of prominent spiral arms or a central bar. The galaxy exhibits a slight color gradient, appearing bluer towards the center and gradually becoming redder in the outer regions. This could indicate a higher concentration of younger, hotter stars in the core, with older stellar populations dominating the outskirts. There is no obvious signs of recent or ongoing major mergers or tidal disturbances, but potentially some signs of minor disturbance.
