This galaxy exhibits a generally elliptical morphology, appearing relatively smooth and concentrated. The core region displays a strong luminosity, suggesting a high stellar density and potentially the presence of a supermassive black hole. Moving outwards from the core, the light gradually diminishes. There is a slight flattening to its shape, indicating a possible deviation from a perfect sphere. The galaxy has a distinct color profile, with the central region showing redder hues which shift toward bluer tones in its outer regions. This may indicate ongoing star formation or a younger stellar population in the outskirts compared to the older stars concentrated in the core. No obvious spiral arms or bar structures are discernible from the image. There is no apparent major merger activity or significant tidal disturbance.
