The galaxy presents as a flattened, elongated structure, suggesting a possible elliptical morphology or a disk galaxy viewed at an oblique angle. The central region exhibits a bright, concentrated luminosity, indicative of a dense stellar population, possibly an active galactic nucleus or a bulge-dominated system. The galaxy appears to have a smooth overall texture with no distinct spiral arm structure visible, which would be consistent with an elliptical galaxy. The color is generally red/yellow, implying an older stellar population with low star formation rate. There is some evidence of faint, extended features or a diffuse halo surrounding the central core. The overall structure appears relatively undisturbed, without any major signs of recent mergers or tidal interactions.
