The galaxy presents as a flattened, elliptical form, strongly suggesting a spheroidal morphology seen nearly edge-on. The central region appears significantly brighter and exhibits a yellowish-white hue, which might indicate an older stellar population dominating this region. Fainter blue regions are visible on the outer edges. These bluer tones may indicate more recent star formation occurring in the disk. The galaxy exhibits a cigar shape. There's little evidence of spiral arms or significant dust lanes. The overall appearance suggests a relatively smooth light distribution. There appears to be no significant interaction or merging events presently occurring, though some minor asymmetry could suggest previous gravitational disturbance.