The galaxy presents a predominantly smooth morphology, exhibiting characteristics of an early-type system. It displays a central bulge, likely composed of an older stellar population, which appears roughly spherical. The light from the galaxy shifts towards the red end of the spectrum. Faint hints of spiral arms are visible, suggesting it could be an early-type spiral galaxy with a significant bulge component. There may be a possible merging event occurring. The overall structure is somewhat disturbed and asymetrical, indicating some kind of interaction. A fraction of bluer colors are seen in the galaxy indicating ongoing star formation.
