The galaxy presents as an elliptical morphology, appearing smooth and relatively featureless. Its shape is elongated, more akin to a cigar than a perfect sphere. The central region exhibits a concentrated luminosity, indicating a significant stellar density. Proceeding outwards from the core, the light gradually diminishes. There is a slight colour gradient from the core to the outer regions, the central bulge appears somewhat yellower, transitioning to a bluer hue in the outskirts. There is no apparent active galactic nucleus. No prominent spiral arms or significant dust lanes are discernible. The galaxy appears to be relatively isolated, with no immediately obvious signs of major interactions or mergers.
