The galaxy presents a generally smooth morphology. It is relatively compact, with a concentrated central region. The light distribution suggests a radial decline outwards from the center. The color profile indicates a yellowish-white hue, potentially suggesting an older stellar population or significant dust obscuration. There appears to be minor asymmetry or a subtle tidal feature. There is no obvious indication of a spiral arm structure or a distinct galactic disk. Overall, the visual characteristics appear consistent with a lenticular galaxy, potentially undergoing a minor interaction.
