The galaxy appears as a slightly elongated spheroid with a smooth, diffuse light distribution, indicative of an early-type morphology. A central, bright bulge dominates the structure, exhibiting a yellowish-orange hue. This coloration suggests an older stellar population within the bulge, potentially composed of evolved red giant stars. A fainter, less defined region extends from the primary bulge, possibly representing a diffuse stellar halo. There is indication of a potential merging event or at least gravitational interaction with a smaller companion galaxy located nearby. This companion is bluer in color. The overall structure shows some degree of disturbance, deviating from a perfectly smooth profile, which might be attributed to a recent or ongoing merger activity.
