This galaxy presents a flattened, elliptical morphology, exhibiting a smooth, diffuse light distribution that suggests it may be an early-type galaxy. The core is bright and concentrated, indicating a high stellar density, possibly with a supermassive black hole at the center. Surrounding this core, a faint, extended halo can be discerned, contributing to the overall ellipsoidal shape. There is evidence of a weak disk structure, though no distinct spiral arms are observed. The galaxy appears inclined relative to our line of sight. The color gradient suggests the presence of older stellar populations, and ongoing, albeit weak star formation, is not ruled out. There are no indications of significant tidal disturbances or interactions with other galaxies in its immediate vicinity.
