The galaxy appears as a relatively smooth, centrally concentrated object with a slight elongation. The central region displays a brighter, more compact core, possibly indicative of an active galactic nucleus or a dense stellar population. A faint, diffuse halo surrounds the central region, exhibiting a subtle blueish hue. This suggests the presence of younger, hotter stars within the outer regions, potentially indicating recent or ongoing star formation. There appears to be a slight disturbance in the morphology of the outer disk, and a subtle feature on one side of the galaxy might indicate a minor interaction or tidal disturbance. The overall structure suggests a galaxy transitioning from a more disk-dominated system to a spheroid, with a significant fraction of its stars residing in a smooth, spheroidal component.
