The galaxy presents as a spiral type, oriented roughly face-on with a slight inclination. Evident are spiral arms exhibiting a somewhat flocculent structure, delineated by regions of blue color indicative of ongoing star formation. These regions appear somewhat patchy in their distribution. The central bulge is prominent and appears relatively bright and smooth, suggesting an older stellar population. A bar structure is potentially present but is not well-defined. The overall color suggests a moderate level of star formation activity, placing it somewhere between a passive elliptical and a vigorously star-forming spiral. There is no strong evidence of a major ongoing merger, although there may be some minor disturbances in the disk possibly indicating minor interactions. The morphological type is likely an intermediate spiral, potentially an SBc type.