The galaxy presents as a relatively smooth, elliptical form, exhibiting a high degree of central concentration. The color profile is generally consistent across the galaxy, with a dominant yellowish hue in the central region, suggestive of an older stellar population and reduced levels of on-going star formation. There is subtle gradient towards greener tints in the outskirts, which may indicate some residual star formation or a difference in stellar population composition. The overall structure shows no readily apparent signs of significant tidal disturbance or ongoing merger activity, although a very slight asymmetry cannot be ruled out.
