The galaxy presents as a centrally concentrated object, exhibiting a roughly elliptical morphology with a relatively smooth appearance. There is a bright, yellowish core which may suggest an older stellar population or the presence of an active galactic nucleus. Surrounding this core is a more diffuse, bluish halo. The lack of distinct spiral arm structures or prominent dust lanes suggests this is likely a lenticular or elliptical galaxy. The subtle color gradients suggest the presence of some ongoing star formation, particularly in the outer regions, but at a low rate. The overall light distribution is centrally dominant, tapering off smoothly into the surrounding background. There do not appear to be any significant tidal features or morphological disturbances indicative of recent major mergers, although a small distortion or minor disturbance may be present.
