The galaxy presents as a centrally concentrated object with a generally smooth morphology. There is an apparent elliptical shape but the profile is fairly round. The central region displays a bright, yellowish-white core, suggestive of an older stellar population. Moving outwards, a subtle blue halo becomes visible, possibly indicative of ongoing, though not necessarily vigorous, star formation in the surrounding region. No distinct spiral arms or bar structures are readily apparent. Slight asymmetries may suggest minor gravitational interaction with another object in the past, but there is no clearly defined merger activity occurring at this time. Overall, it exhibits characteristics consistent with an early-type galaxy, possibly an elliptical or lenticular type, at a significant distance.
