The galaxy presents as a slightly inclined disk galaxy. The central bulge is prominent and exhibits a bright, concentrated luminosity. The disk component shows a smoother texture compared to a spiral galaxy, with a gradual decline in luminosity from the bulge outwards. There is a hint of bluer light in the disk suggesting some recent star formation, but the galaxy appears more evolved, leaning towards an intermediate type. The overall shape is elongated, with a ratio of major to minor axis indicating a moderate degree of flattening. There are no obvious signs of strong disturbances or tidal features, which could suggest recent mergers or interactions.
