The galaxy presents as an elongated, cigar-shaped structure. Its overall light distribution appears relatively smooth, with a concentration of luminosity towards the center, suggesting the presence of a galactic bulge. There is a subtle color gradient visible, shifting from a warmer, redder hue in the central regions to slightly bluer tones at the periphery. This could indicate older stellar populations concentrated centrally, with younger, hotter stars populating the outer regions. There is no obvious spiral arm structure or strong dust lane obscuration. The overall morphology suggests an elliptical galaxy viewed from a significant angle, or potentially a lenticular galaxy with a very weak disk component. There are no obvious signs of tidal disturbances or ongoing mergers, suggesting the galaxy is relatively undisturbed.
