This galaxy presents a complex morphology. The central region exhibits a bright, yellowish-white core, suggestive of an older stellar population or a significant concentration of dust. The overall shape appears to be somewhat elliptical, with a diffuse, extended halo. Some faint, bluer regions can be observed along the periphery of the galaxy, possibly indicative of ongoing, but relatively low, star formation activity. There is a subtle suggestion of tidal disturbances or interactions. Possible signs of minor mergers are visible.
