This galaxy presents a generally smooth morphology. The central region exhibits a high concentration of light, appearing nearly spheroidal in shape. The light gradually diffuses outward, fading into a faint halo. A slight elongation is observed, hinting at a departure from perfect circularity, and leaning more towards an in-between shape. There is very little evidence of strong tidal features, or signs of a major merger. It's possible there are signs of minor disturbances. The colour profile suggests a relatively evolved stellar population, especially in the central bulge, with a bluer component in the more extended outer regions, which could indicate ongoing star formation. The galaxy is likely a massive system, with indications of significant star formation.
