The galaxy presents a generally smooth appearance, exhibiting a slightly elongated, disk-like structure. The central bulge region appears more concentrated and exhibits a yellowish-white hue, suggestive of an older stellar population. Fainter, bluer light extends outwards from the central region, hinting at the presence of a stellar disk with ongoing or recent star formation. There are minor disturbances suggesting the possibility of a past or ongoing interaction with another celestial body. 
