The galaxy presents a generally smooth and rounded morphology. There is a distinct central bulge region that appears quite luminous and concentrated. The color of the central region is skewed toward the redder part of the spectrum, indicating an older stellar population. There is a subtle transition in color and luminosity as one moves outward from the central bulge into the galaxy's outer regions, where the light appears less intense. The galaxy exhibits minimal evidence of spiral arms or other distinct features; rather, the light is diffusely spread. There is no indication of active star formation or significant dust lanes present in this image. The overall shape is close to circular, with minimal elongation or distortion. No signs of tidal interactions or ongoing mergers with other galaxies are visible.
