The galaxy presents an overall elliptical morphology, elongated with a cigar-like appearance. The central region displays a concentration of light, appearing as a smooth, yellow-tinged bulge. Moving outward from the core, the light gradually fades into a more diffuse halo. The outer regions exhibit a subtle blue hue, potentially indicative of younger stellar populations or ongoing star formation, but the overall smooth appearance suggests a galaxy with a significant fraction of older stars. There is no distinct dust lane or spiral arm structure visible; instead, the light distribution remains relatively smooth across the galaxy’s extent. There is no sign of any major galactic merger or significant disturbances in the structure.
