The galaxy presents as a moderately luminous object with a generally smooth morphology. The overall shape appears elliptical, showing a high degree of roundness in its visible structure. There is a subtle color gradient, with the central region exhibiting a warmer, more yellow-orange hue, potentially indicative of an older stellar population or dust obscuration. Fainter blue-ish or green-ish emissions appear to extend slightly from the core, perhaps representing areas of more recent, albeit subdued, star formation. There is no obvious spiral arm structure or bar feature discernible in this image. The slight irregularities or distortions at the edges may be from interactions with other objects nearby.
