The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated, bright central bulge. The light profile suggests a gradual decline in intensity from the core outwards, indicating a lack of distinct spiral arms or significant substructure. The color gradient shows a yellowish-white core, transitioning to a bluer hue in the outer regions, potentially indicating a mix of older stellar populations in the center and younger, star-forming regions further out, though the overall color is subdued. The galaxy appears somewhat elongated and exhibits some evidence of minor disturbances in its morphology. The galaxy doesn't present any major mergers, or disturbances which indicate a relatively relaxed state.
