The galaxy appears as a centrally concentrated object with a smooth, diffuse profile. The light distribution suggests an elliptical morphology, characterized by a gradual decrease in luminosity from the core outwards. The color profile indicates a concentration of older stellar populations with minimal dust extinction. There is little evidence of spiral arms, star-forming regions, or major disturbances. Faint, diffuse light extends outwards from the central region, but no distinct features or structures are discernible. The overall appearance suggests a galaxy that is in a relatively quiescent state, with ongoing, low level star formation.
