The galaxy presents as a relatively smooth, disk-like structure with a central bulge. Its shape is elliptical, exhibiting a flattened appearance rather than perfect circularity. There is some evidence of internal structure, specifically a subtle color gradient from the central region outwards. The core appears yellow-white, indicative of an older stellar population. A faint blue halo surrounds the galaxy, possibly signifying regions of more recent star formation. There is no indication of ongoing major mergers, strong tidal features, or significant dust lanes that are obviously present. The overall appearance suggests a relatively evolved system, showing minimal signs of strong disturbances.
