This galaxy appears to be a relatively compact object, approximately elliptical in shape. It exhibits a generally smooth light distribution, though some irregularities are visible. The galaxy's core appears brighter and more concentrated, fading outwards towards its edges. There is evidence of minor disturbances in its structure, possibly indicative of past or ongoing interactions. A subtle elongation is visible, suggesting it is not perfectly spherical. Overall, the galaxy presents a somewhat rounded morphology, with only slight deviations from a circular form. A small fraction of the light distribution seems to be merging with other galaxies.
