The galaxy presents a complex morphology, indicating ongoing or recent interaction. A prominent central bulge is visible, exhibiting a yellowish-white hue, suggestive of an older stellar population. Spiral arms extend from the central bulge, though they appear somewhat disrupted and ill-defined, with indications of active star formation regions that give them a slightly patchy appearance.

A significant tidal tail or bridge is evident extending from the galaxy, indicating a possible gravitational interaction with a merging galaxy. The galaxy system as a whole appears moderately luminous, with a redder overall color. Given the observed features, this galaxy may be classified as a spiral galaxy undergoing a merger event, or perhaps a recent one.
