The galaxy presents an elliptical morphology, exhibiting a relatively smooth and featureless structure. The light distribution is concentrated towards the center, gradually decreasing outwards. The galaxy displays a color gradient, with the central region appearing more yellowish-white, suggesting an older stellar population, while the outer regions exhibit a bluer hue. This could indicate the presence of younger, hotter stars in these areas, or the possibility of some residual star formation.

The shape appears elongated, with the major axis significantly longer than the minor axis. There is no readily apparent evidence of a distinct disk component or spiral arms. The galaxy's overall structure does not show signs of any major ongoing mergers or significant disturbances.
