This galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears to be largely spheroidal with minimal discernible features such as spiral arms or a prominent disk. There may be a slight flattening that indicates this galaxy isn't completely spherical. The color profile shows a redder central region transitioning to bluer hues in the outer halo or envelope. This suggests the presence of an older stellar population concentrated within the galaxy's core, with relatively younger star formation in the periphery. No major disturbances or ongoing merger events are obviously visible within this image, which suggests that the galaxy is likely relatively relaxed dynamically. The overall smooth appearance indicates an elliptical galaxy.
