The galaxy appears to be a spiral galaxy viewed nearly edge-on, possessing a prominent disk. The central bulge is noticeably brighter and exhibits a yellowish-orange hue, suggestive of an older stellar population dominated by redder stars. The disk displays a bluer tint with less prominent dust lanes visible along the plane, likely due to the edge-on perspective. There is little evidence of significant ongoing star formation, as indicated by the absence of bright blue regions associated with young, massive stars. The overall morphology suggests a relatively evolved system, lacking major disturbances or interactions with other galaxies. The galaxy's disk is elongated, presenting an aspect ratio consistent with a flattened structure viewed at a high inclination.
