The galaxy appears to be a relatively smooth, elliptical galaxy, with a generally spheroidal shape, though it is not perfectly circular. There is some evidence of a very slight elongation. The galaxy exhibits a color gradient, with a central region that is more yellowish-white, indicative of an older stellar population. Moving outward, the galaxy becomes slightly redder, particularly at the top edge. This suggests the presence of some dust or older stars further from the galactic center. There are no obvious spiral arms or disk-like structures visible. There's also a small hint of blue concentrated near the center, which might indicate the presence of some ongoing, but not substantial, star formation. Overall, the galaxy appears to be a fairly massive system. The image suggests that the galaxy may be undergoing, or may have recently undergone, some form of disturbance or interaction, though it is not extreme. There's only minor evidence of a merger event.
