The galaxy presents an elliptical morphology, appearing largely smooth and featureless. Its central bulge is prominent, exhibiting a concentrated luminosity gradient towards the core. The color profile suggests an older stellar population, with a yellowish-red hue dominating the central region. The outer regions display a fainter, more diffuse light distribution, indicative of a gradual decrease in stellar density. There is no clear evidence of spiral arms or significant dust lanes. The overall structure suggests a relatively evolved system, possibly with minimal ongoing star formation. There is a slight elongation, but it is mostly round in shape. No clear evidence of major mergers.
