The galaxy presents a flattened disk-like morphology, observed at a moderate inclination. Evident spiral arm structures are present, though somewhat ill-defined and flocculent. A distinct central bulge is visible, appearing relatively bright and concentrated. The galaxy exhibits a range of colors, with a yellowish core potentially indicating an older stellar population in the bulge, transitioning to bluer hues in the outer spiral arms which may suggest the presence of younger, hotter stars associated with active star formation. There are indications of some morphological disturbances, possibly tidal interactions or the remnants of a minor merger event, contributing to the galaxy's somewhat irregular overall structure.
