The galaxy presents as a relatively smooth and moderately elongated structure. The central region exhibits a concentration of light with a slightly reddish hue, suggesting an older stellar population. Progressing outward from the core, the galaxy transitions to a bluer color, which likely corresponds to younger stars. There are some slight indications of faint arm-like structures, however, the disk is not clearly defined. It appears that there has been a period of low-level star formation. There is no indication of any recent or major merger activity.
