The galaxy appears to be an intermediate-type galaxy, possibly exhibiting characteristics of both elliptical and spiral galaxies. The overall structure is somewhat diffuse with a moderate degree of central concentration but lacking a well-defined nucleus. There are hints of spiral arm features, but these are not sharply defined and appear somewhat disrupted. The galaxy exhibits a subtle bluish tint in its central regions, suggestive of ongoing star formation, with the outer regions appearing slightly redder, which could indicate an older stellar population. There is possible minor tidal disturbance on the sides. Overall, the galaxy appears to be experiencing some sort of ongoing interaction or internal dynamical process.
