The galaxy exhibits an overall elliptical morphology, appearing largely smooth and spheroidal in shape. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. There is little evidence of spiral arm structure or significant dust lanes. The color profile suggests a higher concentration of older stellar populations, particularly near the core, which appears more yellow/red. Fainter, bluer light is present in the outer regions. Overall, the galaxy seems to be a relatively evolved system, consistent with a classification as an elliptical galaxy.
