The galaxy presents a predominantly smooth morphology. A bright central bulge is observed, emitting strongly in the g, r, and z bands, indicative of an older stellar population. There is a slight elongation in the galaxy's shape along its north-south axis, suggesting it is not perfectly spherical. The overall color profile indicates a lack of substantial ongoing star formation, with a redder color suggesting evolved stellar populations dominate. Possible minor disturbances or faint tidal features are suspected extending from the main body, though the resolution is not sufficient to confirm. The galaxy does not present a clear spiral structure or a prominent disk.
