This galaxy exhibits a roughly elliptical morphology. A bright, concentrated central region is observed, suggestive of a significant stellar population density or active galactic nucleus. The core is surrounded by an extended, less intense halo. The halo appears complex, showing some asymmetry and potential disturbances in its structure, possibly indicating past or ongoing interactions. Overall, the galaxy's light profile suggests a relatively smooth distribution, with a higher concentration toward the center. Evidence of a disk or spiral arms are absent. It's possible the observed structure is the result of a recent minor merger event, however a significant portion of the morphology appears smooth. The distribution of light across the galaxy exhibits some color variations, with the central bulge appearing more bluish than the outer regions, indicative of varying stellar populations or differing dust content. The image suggests a system in a state of transition or potential interaction.
