The galaxy presents a largely smooth, elliptical morphology. It exhibits a central, bright, yellowish core, suggesting an older stellar population. The overall shape appears moderately flattened, falling somewhere between a perfectly spherical and highly elongated form. There's a hint of a disk-like structure, though it's very faint and not well-defined. There's no visually apparent evidence of ongoing major mergers or significant tidal disturbances, but subtle asymmetries and minor disturbances cannot be ruled out based on the current image resolution. The galaxy appears relatively isolated, with no large interacting neighbors within the immediate field. Star formation is likely present, but appears to be at a relatively low rate.
