The galaxy presents a largely smooth morphology, with a dominant spheroidal component. It appears generally rounded in shape, though with slight deviations from perfect circularity. The central region exhibits a strong concentration of light, appearing significantly brighter and potentially indicative of an active galactic nucleus or a dense stellar population. A faint disk structure might be present within the brighter area. The outer regions are more diffuse, showing a gradual decrease in luminosity. Irregular features, possibly indicative of tidal disturbances or ongoing merger activity, are noticeable, though they are not dominant. These irregularities suggest a complex gravitational interaction history, potentially influencing star formation within the galaxy. Color gradients are subtle, but there's a suggestion of redder hues in the central regions compared to the bluer, fainter outskirts, possibly indicating older stellar populations towards the center and younger populations in the outer regions.
