The object is a spiral galaxy exhibiting a clear disk structure. The galaxy's inclination is such that it is viewed at a shallow angle, but not fully edge-on, allowing for some observation of its spiral arm structure. The spiral arms appear somewhat flocculent and patchy, with brighter regions suggestive of active star formation along their length. A distinct central bulge is visible, though it does not appear to be the dominant feature of the galaxy's overall morphology. The presence of a bar is suspected, based on the rectangular shape of the bulge. Overall, this galaxy presents itself as a well-defined spiral, with ongoing star formation. The color suggests intermediate age stars in the arms. Some possible minor disturbances could be present.
