The galaxy presents as a moderately inclined disk system, likely a spiral galaxy viewed somewhat face-on. The central bulge is prominent and appears smooth with a bright core, suggesting a relatively older stellar population dominating this region. Fainter spiral arms are detected. The spiral arms appear relatively tightly wound. There are hints of clumpy star formation regions scattered along the spiral arms, characterized by a bluer color. The overall color of the galaxy suggests ongoing, but perhaps not exceptionally vigorous, star formation. The galaxy does not exhibit any obvious signs of a recent major merger event. However, there might be minor tidal disturbances or irregularities in the outer disk, indicative of possible minor interactions or accretion events.
