The galaxy presents as a central, moderately bright core that appears nearly smooth in texture. Extending outward from this core is a fainter, elongated structure. Within this extended feature, there are hints of irregular dust lanes or spiral arm segments, particularly on one side of the galaxy, giving it a slightly disturbed appearance. The overall color profile suggests an older stellar population, dominated by redder wavelengths, with some indication of recent star formation concentrated in localized regions. The elliptical shape of the galaxy is elongated with a notable deviation from a perfect circle. The galaxy seems to be undergoing some sort of minor merger as a result of its distorted shape.
