The galaxy presents as an elliptical or lenticular morphology, exhibiting a smooth, concentrated central bulge. The light from the bulge is a yellowish hue, indicating a population of older stars. Moving outward from the core, the galaxy displays a flattened disk-like structure. The disk shows hints of spiral arm structure that is not fully resolved. These arms are tinged with a faint bluish color, suggesting the presence of younger stars. The overall color distribution points to suppressed ongoing star formation, likely transitioning to a more quiescent state. The galaxy exhibits a moderate degree of inclination, presenting an elongated, cigar-like shape. Faint indications of tidal features or minor disturbances are visible in the outer regions, suggesting past or ongoing interactions with other galaxies.