The galaxy appears as a somewhat concentrated, luminous object with a notable red-shifted color profile. It displays a generally smooth morphology with a suggestion of a disk-like structure viewed at an oblique angle. There is evidence of some internal structure, possibly including areas of active star formation evidenced by the red coloration. The galaxy's shape is neither perfectly spherical nor highly elongated, exhibiting an intermediate form. There is faint disturbance within the galaxy, maybe an indication of past or ongoing minor mergers or tidal interactions.
