The galaxy presents as a centrally concentrated object, generally ellipsoidal in shape. A bulge component is clearly dominant and exhibits a yellowish hue, suggesting an older stellar population. Surrounding this central region, a fainter, bluer disk component is detected, though it appears relatively smooth and lacking in significant spiral structure. Subtle variations in color are observed, with the outer regions of the disk showing a slightly bluer tint compared to the inner bulge, indicative of ongoing or recent star formation. No strong tidal features or signs of recent major merger events are apparent. The overall morphology indicates a galaxy somewhere on the spectrum between a lenticular and an elliptical galaxy, possibly an early-type spiral with a weakly defined disk.
