The galaxy presents as a somewhat compact, elliptical-like system with a bright, concentrated nucleus. A distinct, yellowish hue dominates the central bulge region, suggesting an older stellar population and potentially a low rate of recent star formation. As seen, the light is more red than blue.

Distortions in the galaxy's disk region or arm structures, along with indications of tidal tails or disturbed morphology are present. This suggests possible interactions or mergers with a smaller galaxy or companion system. The color variation is also evidence of star formation.

Overall, the galaxy appears to be at an intermediate stage of evolution, exhibiting properties of both elliptical and spiral galaxies, with signs of past or ongoing interaction influencing its morphology and stellar populations. The light is strongly red-shifted.
