The galaxy presents as a moderately luminous object with a discernible, albeit somewhat ill-defined, disk structure. The central region exhibits a high concentration of light, suggestive of a prominent bulge or nucleus. The color profile indicates a redder hue in the central region, potentially indicative of an older stellar population or increased dust obscuration. Moving outward from the center, a slight bluer tint is observed, possibly due to younger stars and lower levels of dust extinction.

There appears to be some subtle asymmetry in the galactic disk, possibly indicating past or ongoing interactions. No spiral arm structures are clearly visible, and the galaxy seems to be relatively smooth. This does not exclude subtle features, however. The galaxy presents an overall elliptical shape, but it does not show a distinct halo in the visible light. 
