The galaxy appears to be a relatively smooth, elliptical or lenticular type, exhibiting a concentrated central bulge and a faint, diffuse halo. It is yellowish in color, suggesting an older stellar population dominated by evolved stars. There is no evidence of strong spiral arm structures or significant dust lanes, although some faint, subtle features might be present within the extended halo. The morphology is generally consistent with a galaxy that has largely ceased active star formation, with a smooth distribution of light and minimal signs of recent disturbances or mergers. The galaxy presents as moderately luminous, with a well-defined core.
