This galaxy appears to be a spiral galaxy observed edge-on, presenting a highly elongated profile. The central bulge is prominent, exhibiting a yellowish-orange hue, suggestive of an older stellar population. The disk appears thin, and is also of a yellow-orange hue. The dust lane is not obvious. There are two small, moderately bright sources in the disk that may be locations of star formation. Based on the morphology, this galaxy does not appear to be undergoing a major merger or significant tidal disruption.
