The galaxy presents as a slightly elongated, ellipsoidal structure. The light distribution is relatively smooth, suggesting a lack of prominent spiral arms or significant dust lanes. The core exhibits a diffuse glow, brighter than the surrounding galactic halo. The overall color is a somewhat red hue, indicative of an older stellar population and moderate dust extinction. There appears to be no signs of active galactic nuclei activity or a recent major merger event. Minor distortions in the galactic disk suggest some tidal interactions or minor disturbances from smaller galaxies, potentially hinting at ongoing hierarchical galaxy formation. The estimated size is about 6 kpc across. There is a low but present rate of star formation within the galaxy.
