The galaxy presents a generally smooth appearance, with a bright, concentrated central bulge that appears roughly circular. The overall color profile suggests a relatively old stellar population, with a yellowish hue dominating the bulge and inner regions. There is a faint disk structure surrounding the bulge, but it is poorly defined and lacks prominent spiral arms. Subtle color variations within the disk suggest potential regions of ongoing or recent star formation, possibly characterized by slightly bluer patches. There may be a minor asymmetry in the outer regions of the disk, suggesting a possible gravitational interaction or minor disturbance. The galaxy appears relatively isolated and unperturbed, exhibiting no major signs of ongoing merging activity.
