The galaxy presents a mostly smooth morphology with a slightly elongated shape. The central region exhibits a concentrated, bright core, suggesting a high density of stars and potentially a supermassive black hole at its center. The color of the core appears yellowish-orange, which would indicate a population of older, redder stars. Extending outwards from the core, there's a faint, diffuse disk or halo-like structure. This outer region shows some subtle color variations, with hints of bluer tones, possibly indicating regions of ongoing star formation. The overall structure appears relatively undisturbed, showing no signs of major mergers or tidal interactions.
