The galaxy presents as a single, somewhat amorphous body with a dominant, concentrated central bulge. The light distribution appears relatively smooth and featureless across the galaxy, suggestive of an elliptical morphology or a late-stage merger. There is a subtle elongation, though the overall shape appears close to round. The core of the galaxy exhibits a slightly more intense concentration of light compared to its outer regions. The color is slightly redder overall with a yellow center, consistent with an older stellar population and relatively low levels of current star formation. Evidence of minor tidal disturbances may be present in the form of faint, extended structures in the outskirts, though this is not definitive. The galaxy appears fairly massive. There is strong evidence of a merger event.
