This galaxy presents as a relatively compact, elliptical or lenticular system. The central region exhibits a high concentration of light, appearing bright yellowish-white, suggestive of an older stellar population. Moving outward from the core, the light intensity gradually decreases, exhibiting a smooth profile with little evidence of distinct spiral arms or significant dust lanes. The overall shape is somewhat elongated but largely consistent with a spheroid. There are subtle hints of a faint, diffuse halo extending beyond the main body of the galaxy, but no clear signs of recent or ongoing major merger events. The lack of blue color suggests a low rate of active star formation within this galaxy. Slight asymmetry is seen in the halo.
