The galaxy appears to be an elliptical galaxy, characterized by a smooth, spheroidal morphology. There is little indication of spiral arms or a distinct disk structure. The central region displays a high concentration of light, suggesting a dense nucleus. A radial color gradient is observed, with the core exhibiting a yellow-red hue. This is surrounded by a more diffuse region with subtle blue-green tones, perhaps indicating the presence of a younger stellar population at the periphery. The overall structure suggests a relatively evolved system, with a dominant older stellar population, but may also include pockets of ongoing star formation. There is no evidence of significant tidal disturbances or interactions with neighboring galaxies.
