The galaxy presents as a lenticular system viewed nearly edge-on. Its morphology exhibits a bright, prominent bulge surrounded by a relatively faint and elongated disk. The bulge appears smooth and well-defined, potentially indicating an older stellar population. The disk is relatively thin, suggesting a high inclination angle. The lack of visible dust lanes or distinct spiral arms suggests a system with little ongoing star formation. The galaxy appears to be relatively undisturbed, showing no signs of recent mergers or significant tidal interactions. The overall color profile indicates a mix of stellar populations, with the central bulge appearing more yellow/orange and the disk having a bluer tint, albeit subtle. 
