The galaxy presents a smooth, largely featureless morphology. It exhibits a centrally concentrated, roughly elliptical shape. The central region displays a bright, almost stellar-like core, suggesting a possible active galactic nucleus or a dense concentration of stars. Moving outwards from the core, the light fades gradually. There's a slight elongation, implying the galaxy is not perfectly spherical, but more of a flattened spheroid. The color profile appears to be predominantly redder/yellower, which could indicate an older stellar population with less ongoing star formation. Subtle hints of blue suggest there is still some presence of younger, hotter stars.
