The galaxy exhibits a roughly elliptical morphology, appearing somewhat elongated. The central region presents a bright, concentrated core, possibly indicating an active galactic nucleus or a dense concentration of stars. The color profile of the galaxy suggests a mix of stellar populations; the central core appears more yellow/white, indicative of older, redder stars, while the outer regions show a bluer hue, suggestive of younger, hotter stars and ongoing star formation. Faint extensions of light are visible, possibly tidal tails or faint spiral arm structures that are undergoing disruption. There are hints of minor disturbances in the galaxy's structure, it does not appear to be a perfectly symmetrical, undisturbed system. The overall light distribution appears relatively smooth, though with subtle irregularities that warrant further investigation.
