The galaxy presents an overall elliptical morphology, appearing elongated with a cigar-like shape. The central region exhibits a concentrated, bright core, suggesting a higher density of stellar populations. A gradual decrease in luminosity is observed from the center outwards, forming a diffuse halo. The color profile indicates a generally redder hue in the core, possibly due to older stellar populations, while the outer regions show a slightly bluer tint, which may indicate the presence of younger stars or ongoing star formation. There is little to no indication of spiral arm structure or significant dust lanes. The overall smooth appearance suggests a relatively relaxed system with minimal signs of recent mergers or major disturbances.
