The galaxy presents as a relatively smooth, round structure, exhibiting a concentrated central bulge that graduates outward into a more diffuse halo. There is a lack of clear spiral arm structure or distinct features, suggesting a later-type morphology. Subtle color variations indicate some star formation, but at a low rate. There are suggestions of minor disturbances, perhaps from small accretion events. The galaxy does not appear to be actively merging with any major companions, instead presenting as an isolated system.
