The galaxy presents a relatively smooth and elliptical morphology, appearing nearly circular. The light distribution is centrally concentrated with a bright, compact core, possibly indicative of an active galactic nucleus or a region of intense star formation. The galaxy's color profile suggests a bluer hue in the central regions, transitioning to redder tones in the outer parts of the main body. There is no obvious spiral structure, though the data indicates a small chance of merging activity. The overall structure suggests a potentially quiescent system with ongoing star formation.
