The galaxy presents an overall disk-like morphology, observed at a near edge-on inclination. A central bulge is apparent, exhibiting a concentrated luminosity gradient. The color profile suggests a complex stellar population; the bulge region appears yellower, indicative of older stars, whereas the disk is bluer, suggesting more recent star formation. The disk shows some evidence of internal structure, possibly spiral arm segments, although the resolution limits detailed assessment. There appear to be some dust lanes present, which is consistent with the disk. There is no evidence of a major merger. However, there might be signs of a minor interaction or some disturbance in the disk morphology.
