The galaxy presents as a relatively smooth, disk-like structure viewed at an oblique angle. There is a distinct central bulge exhibiting a yellowish-orange hue, suggestive of an older stellar population. The surrounding disk appears less structured, with a bluer color gradient as it extends outward from the bulge, indicating the presence of younger, hotter stars and potentially ongoing star formation. The galaxy displays an elliptical morphology, more elongated than circular, with a hint of minor asymmetry. The absence of prominent tidal features or other major disturbances suggests the galaxy is relatively isolated, with no ongoing or recent major merger events.
