This galaxy exhibits a generally smooth morphology, though it appears to show faint features of a possible disk. A brighter, yellowish central bulge is clearly present. Surrounding the bulge, there's an extended, slightly irregular halo of bluish light. This halo suggests the presence of a younger stellar population and ongoing star formation. There's no strong visual evidence of a major ongoing merger, though subtle disturbances in the outer regions cannot be ruled out. The galaxy appears relatively isolated, with no other immediately interacting galaxies visible in the vicinity. The overall shape is somewhat elliptical, with the long axis roughly oriented vertically.
