The galaxy presents a generally smooth morphology, appearing largely featureless at this resolution. Its shape is predominantly round, with a slight elongation that doesn't significantly deviate from circularity. A concentration of light is observed toward the center, suggesting the presence of a galactic bulge. The light is most intense at the very center. There are no visible signs of tidal tails, merging events, or major disturbances.

Color gradients suggest some variation in stellar populations throughout the galaxy. The core exhibits a more yellowish hue, potentially indicative of older, redder stars. The outer regions show a subtle shift towards bluer tones, which could point to more recent star formation activity or a population of younger, hotter stars. However, the overall star formation rate appears relatively low. The galaxy does not show a prominent disk structure.
