The galaxy exhibits a generally elliptical morphology with a moderate degree of smoothness. There is evidence of a possible disk structure, though not sharply defined. Features suggest it could be experiencing some gravitational interaction; a minor disturbance seems plausible. There is a hint of a merger in the galaxy's morphology. The galaxy displays a color gradient from a brighter, central region to fainter outer areas. The core appears to be a slightly redder hue, transitioning to a bluer color in the more diffuse, surrounding regions. The overall color suggests a mix of stellar populations, where there may be both younger, bluer stars and older, redder stars present.
