The galaxy presents a disk-like morphology, viewed at an angle, although not perfectly edge-on. A spiral structure is clearly discernible, characterized by arm segments. The central bulge appears moderate in size. The arms have a tightly wound appearance. There may be evidence of a bar structure crossing the central region of the galaxy. No signs of major mergers or significant tidal disturbances are immediately obvious. The overall color profile suggests a relatively mature stellar population within the bulk of the galaxy. Some regions of bluer light are seen in the arms, possibly indicating areas of recent star formation.
