The galaxy presents a generally smooth morphology, with a dominant central bulge. The light distribution suggests a concentration of older stellar populations within the bulge, exhibiting a yellow-orange hue. Faint blue colors can be seen in the outskirts, which could be evidence of recent or ongoing star formation activity within a disk-like structure or spiral arms. However, these features are not clearly defined, indicating the galaxy is most likely an elliptical or lenticular galaxy. The outer regions appear to be fading out, and the shape of the galaxy is generally round, although not perfectly so. There are no indications of a major ongoing merger or significant tidal disturbances that might be influencing the overall structure, however there could be a small companion on the left side of the galaxy.
