The galaxy presents a largely featureless morphology, appearing as a single, somewhat symmetrical object. The light distribution suggests a concentrated central region, possibly indicating a bulge component. The overall form is neither perfectly spherical nor highly elongated, exhibiting an intermediate shape. There is no obvious evidence of spiral arms or a distinct disk structure.

The galaxy exhibits a color gradient, appearing slightly yellower in the central regions, transitioning to a bluer hue in the outer parts. This might suggest ongoing, yet modest star formation activity. There is no immediately apparent sign of strong tidal interactions, or major mergers. Small structural disturbances cannot be ruled out at this level of image resolution.
