The galaxy appears to be an elliptical galaxy, characterized by a smooth, symmetrical light distribution. The galaxy exhibits a concentrated central bulge, with the light intensity decreasing gradually towards the outer regions. There is a subtle color gradient, with the core appearing more yellow-orange, suggesting an older stellar population dominated by red giant stars. The outer regions appear slightly bluer, which could indicate a small population of younger, hotter stars. The overall morphology suggests that the galaxy is well-relaxed and potentially a product of previous galaxy mergers. There is no obvious indication of spiral arms or a prominent disk structure. Based on the color and morphology, this galaxy is likely relatively massive. Although generally smooth in appearance, there may be some minor structural disturbance or tidal features present, suggesting a possible minor interaction event in its past.
