The galaxy presents a relatively smooth morphology. Its shape is mostly elliptical, appearing somewhat elongated but not cigar-shaped. The central region exhibits a bright, concentrated luminosity, which gradually diminishes towards the outer edges. There is some suggestion of a slight distortion in the overall structure, hinting at potential interactions or minor disturbances. The color profile appears to be predominantly composed of older stellar populations, with a slightly redder hue at the center, transitioning to a bluer tint in the outer regions. Evidence of spiral arm structure is either absent or unresolved in this image.
