The galaxy appears as a somewhat elongated, disk-like structure. The central bulge exhibits a smooth, concentrated light profile with a yellowish hue, suggesting an older stellar population. Moving outwards from the center, the light becomes slightly more diffuse, with hints of bluer components. Overall, the galaxy presents a moderately inclined orientation relative to the observer. There is no visual evidence of a strong spiral arm structure or prominent dust lanes. The overall impression is of a relatively evolved galaxy, possibly undergoing a low level of star formation. There may be some minor disturbances in the shape, but overall it looks mostly undisturbed.
