The galaxy presents a largely smooth morphology, with a notable lack of distinct spiral arms or a bar. The light distribution suggests an elliptical or lenticular type. It appears somewhat flattened, displaying an "in between" roundness suggesting moderate ellipticity. The core exhibits a concentrated, brighter, and more yellow-ish hue, potentially indicative of an older stellar population. Moving outwards from the core, there's a gradual decrease in luminosity and a shift in color towards slightly greener tones. The edges are diffuse and fade gradually into the background, indicating a lack of sharp boundaries. There's no obvious signs of active merging or major disturbances; the overall structure appears relatively undisturbed. The galaxy does not seem to have much recent star formation.
