The galaxy presents as a moderately inclined, somewhat diffuse spiral, exhibiting a relatively smooth, centralized bulge component. The disk is visible, though it lacks well-defined spiral arm structure, appearing somewhat flocculent. There are hints of blue-ish color in the disk, suggesting the presence of young, hot stars indicative of recent star formation. However, the overall light distribution is dominated by a more yellowish-white hue, implying a stellar population that is a mix of younger and older stars. There is no obvious strong central bar structure, nor is there significant evidence of tidal disturbances or recent merger activity, though some slight asymmetries may be present. The galaxy is moderately compact, with the bulk of its light concentrated in the central regions.
