The galaxy presents a generally smooth morphology, with a concentrated central region. The light distribution suggests a spheroidal shape, though not perfectly circular; there is a slight elongation evident.

Color gradients indicate a possible difference in stellar populations between the central bulge and outer regions. The central region appears more concentrated and exhibits a yellowish-orange hue, potentially indicative of older stellar populations. The surrounding regions display bluer color components, hinting at some presence of younger, bluer stars and possibly ongoing star formation.

There are suggestions of minor disturbances in the morphology. While predominantly smooth, closer inspection suggests a possibility that the galaxy is undergoing a merger with another galaxy.
