This galaxy exhibits a generally smooth morphology, though not entirely featureless. A slight elongation is visible, suggesting it is either an elliptical galaxy or a spiral galaxy viewed at an angle. The central region presents a bright, concentrated bulge, indicating a high stellar density, which is indicative of an older stellar population. The surrounding disk, if present, is faint and less defined. The presence of bluer hues in the outer regions hints at ongoing star formation, though not dramatically so. There appears to be some minor disturbance to the overall smooth shape, possibly due to a minor interaction or merger in the galaxy’s past. The galaxy does not show strong indications of a major merger event.
