This galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution. It is elongated in shape, with a noticeable flattening. The core of the galaxy displays a bright, yellow-white hue, suggesting an older stellar population dominates the central region. This color shifts to a slightly redder tone in the outer regions, perhaps indicating the presence of dust or a slightly younger, redder population of stars compared to the nucleus. There is no evidence of spiral arms or significant dust lanes. The overall smooth appearance suggests that it is not currently undergoing a major merger, with no significant morphological disturbances visible in this image.
