This galaxy exhibits a distinct elongated, cigar-like morphology. The central region displays a bright, concentrated luminosity, indicating a significant stellar population. Moving outward from the core, the light gradually diminishes, forming a smooth halo. There may be faint indication of a disk structure. The overall color is a somewhat blue-ish white, with perhaps a hint of reddening towards the periphery. The smooth appearance suggests an older stellar population and a lack of active star formation. There appear to be no indications of major tidal disturbances or ongoing merger activity.
