The observed galaxy presents as a centrally concentrated object with a generally smooth morphology. The primary body exhibits a near-circular profile, with a slight elongation perhaps inferring some disc structure, but this is not definitively confirmed by this data. The galaxy's core presents a bright, relatively uniform luminosity gradient decreasing outward to fainter regions. There is no prominent central bulge.

The color profile suggests an older stellar population, however there are regions of younger stars. There is one region of very intense, concentrated, bright light that hints at star formation. The overall color of the galaxy appears somewhat yellow, consistent with a population that has undergone significant, but not total, redshifting.

There may be a merging event occurring based on the disturbances to the elliptical shape and differing colors within the same object. There is also a long band of light and color that could be either a tidal tail due to interactions with another object or a disrupted arm.
