The galaxy presents a generally smooth morphology, suggesting it is likely an early-type galaxy. The color profile indicates a redder hue, particularly concentrated towards the galactic center, implying an older stellar population and reduced ongoing star formation. Although partially obscured by the inherent blurring of distant objects, there is subtle evidence of possible arm structures. The galaxy is neither perfectly elliptical nor highly irregular; it could be an intermediate stage between elliptical and spiral. There are no obvious signs of recent major merging events or significant tidal disturbances. The morphology appears relatively undisturbed.
