The galaxy presents as a flattened, elliptical structure. The central region exhibits a bright, concentrated luminosity, suggesting a higher density of stars and potentially a supermassive black hole at its core. Moving outward, the luminosity gradually diminishes, indicating a decreasing stellar density. The overall color appears slightly reddish, which could be indicative of an older stellar population and/or the presence of dust obscuring bluer light from younger stars. There is no apparent spiral arm structure. The galaxy appears relatively undisturbed, with no major signs of ongoing merger activity or tidal distortions. The shape is elongated, approximating a cigar shape, and the galaxy appears smooth, without obvious, distinct features.
