This galaxy presents as a slightly elongated, disk-like structure. It displays a relatively smooth, though subtly textured, appearance without prominent spiral arms or a well-defined bar. The color profile appears somewhat uniform across the galaxy, showing a general concentration in the redder wavelengths with a G-band magnitude suggesting moderate star formation is occurring, but not dominating. There may be only minor distortions in the general structure and no obvious signs of an ongoing major merger, however, there is a slight irregularity that is barely perceivable. Based on the relatively homogenous color and morphology, it could be undergoing a minor interaction. The overall roundness suggests it leans towards an elliptical type, or perhaps a lenticular galaxy seen at a slight inclination, consistent with the lack of prominent features.
