The galaxy presents as an elongated, elliptical structure. Its color profile suggests a dominant population of older stars, indicated by the reddish-orange hue concentrated towards the central bulge. A subtle gradient is observed transitioning to a bluish tint in the outer regions. This may indicate some on-going, yet limited star formation. The galaxy exhibits a relatively smooth morphology with no obvious spiral arm structure or significant dust lane features, although some minor disturbances could be occurring. There is moderate ellipticity to the galactic shape. The galaxy appears reasonably isolated, with no immediately apparent signs of a major ongoing merger.
