This galaxy appears to be of an elliptical morphology, possessing a generally smooth and rounded structure with no discernible spiral arms or a prominent central bulge. The light distribution suggests a relatively uniform stellar population. A subtle color gradient can be observed, transitioning from a warmer, redder hue in the central regions to a slightly bluer tint in the outer areas. There are minor disturbances to the shape that indicate a possible previous minor merger or tidal interaction. Furthermore, a feature to the left of the central body of the galaxy is indicative of a second interacting galaxy. The galaxy appears to be in the early stages of merging with another galaxy. Overall, this galaxy presents as a relatively evolved system, although indications of interactions suggest further evolution is underway.
