The galaxy appears to be a spiral galaxy viewed at a significant inclination. The central bulge is prominent, exhibiting a yellowish hue, suggestive of an older stellar population. Fainter spiral arms extend outwards from the bulge. These arms are relatively tightly wound and somewhat diffuse. There is evidence of some star formation occurring within these arms, as indicated by the bluer, scattered regions. No strong bar feature is observed. The overall morphology suggests this is a galaxy in a relatively quiescent state, with ongoing star formation at a moderate rate. There is no obvious evidence of a major merger or significant tidal disturbance affecting the galaxy's structure.
