The galaxy presents as a moderately luminous object at a redshift of approximately 0.205. Morphologically, it appears to be a relatively smooth galaxy, with a slight elongation, but with some non-uniformity of color distribution.

The central region has a yellow-white hue, which fades somewhat at the edges. There is a hint of a faint, extended halo beyond the main galactic body. Evidence of recent mergers is relatively limited, with no major visible disturbances. The galaxy has an estimated stellar mass likely on the order of 10^10 to 10^11 solar masses.

Star formation is estimated to be moderately suppressed, likely reflecting a transition towards a more quiescent state. The overall morphology suggests a system that could be transitioning from a spiral to an elliptical type, or a low-mass elliptical galaxy.
