The galaxy appears as a relatively bright, centrally concentrated object. The core exhibits a dominant, smooth, yellowish-white glow, suggesting an older stellar population. A surrounding, fainter and bluer halo extends outwards. This outer region seems less uniform, possibly indicating some structural features or irregularities. The overall shape is somewhat elliptical, but with a slight asymmetry. There is no clear evidence of a prominent disk or spiral arms. The galaxy shows some signs of possible disturbance; it looks like a past or ongoing minor merger may have occurred. Based on its blue outer regions and mass estimates, the galaxy is actively forming stars, but at a rate that may not be particularly high compared to its total mass.
