The galaxy presents as a relatively smooth, elliptical-like structure. The core exhibits a concentrated, luminous glow, suggesting a high density of stars in the central region. Moving outward from the core, the luminosity decreases, and a diffuse halo is observed. The galaxy appears elongated, with a cigar-like shape. There is no apparent strong spiral arm structure or significant dust lane obscuration visible. Faint blue-ish hues are observed outside the brighter core, possibly indicating regions of younger stars or ongoing star formation, although at a relatively low rate. Overall, the galaxy appears to be a massive system, likely a evolved galaxy undergoing little to no major merging activity.
