The galaxy presents a generally smooth morphology. Its shape is somewhat elongated, appearing more akin to an elliptical galaxy, although a subtle disk-like feature may be present. The central region is significantly brighter, with an intense yellowish-white hue, suggesting an older stellar population. Moving outwards from the core, the galaxy transitions to bluer colors, hinting at the presence of younger stars and possibly ongoing star formation in the outer regions. There is some asymmetry present, potentially indicating a minor gravitational interaction. There are no obvious signs of a major merger or significant tidal disturbances.
