The galaxy presents as a spiral with a moderate bulge. A distinct disk is visible, exhibiting a slight inclination relative to the observer's line of sight. Traces of spiral arms can be discerned winding outwards from the central bulge, showing some flocculence. The bulge appears yellowish-white, suggesting an older stellar population. The disk has a bluer hue, indicative of ongoing star formation. There appear to be some minor disturbances of the galaxy, indicating a small probability of a merger. Based on the light distribution, the galaxy's shape deviates slightly from a perfect circle, with a Sersic index consistent with a profile between that of a pure disk and a typical elliptical galaxy. Redshift is at 0.075449.
