The galaxy presents as a relatively smooth, centrally concentrated object with a disk-like morphology. The central region appears bright and somewhat spheroidal, possibly indicating a bulge component. Faint spiral arm features are tentatively visible. There may be little star formation occurring, with a dominant older stellar population indicated by the red color of the galactic halo, and a lack of distinct HII regions or bright knots. There is an indication of a slight asymmetry in the shape, possibly hinting at a past minor interaction. The galaxy is relatively isolated in the field, with no clear evidence of major ongoing merger activity.
