This galaxy exhibits a generally smooth morphology, appearing as an elliptical or lenticular type. It displays an elongated, cigar-like shape. The central bulge is prominent, characterized by a bright, concentrated luminosity indicating a high density of older stars. Moving outward from the core, the intensity of light gradually decreases. There is some evidence of a faint, diffused disk component with hints of subtle structure. Overall, the galaxy appears relatively undisturbed, without any obvious signs of a major merger or strong tidal interactions.
