The galaxy presents as an edge-on spiral with a prominent central bulge. The bulge exhibits a concentrated, smooth light profile with a yellowish-orange hue, suggestive of an older stellar population. Faint disk components extend laterally from the bulge, appearing somewhat asymmetrical. The dust lane obscuration is likely present, though difficult to discern, based on the apparent light falloff. Indications of tidal disturbance or merging events are not readily apparent in this image at this resolution. The galaxy exhibits a moderate degree of red shift, with a significant stellar mass. The star formation rate appears to be relatively low.
