The galaxy presents as a disk-shaped structure, viewed at an oblique angle, approaching edge-on. A central bulge is apparent, exhibiting a yellowish-white hue, which suggests a higher concentration of older stellar populations. Fainter regions are located away from the center. These areas show a bluer tint, suggesting the presence of ongoing star formation, although at a low rate. The disk appears somewhat flocculent, with hints of spiral arm structure, though not sharply defined. The galaxy appears relatively smooth, without any major distortions or tidal features suggestive of recent or ongoing major mergers. It has an elliptical form due to its edge-on orientation.
