The galaxy presents a somewhat lenticular appearance, exhibiting a flattened disk-like structure viewed at an oblique angle. A central bulge is visible, characterized by a concentrated, bright luminosity suggesting a high density of stars. The color of the bulge appears to be generally redder than the surrounding disk, potentially indicating an older stellar population with fewer young, hot stars.

The disk shows a smoother texture compared to spiral galaxies, with little evidence of distinct spiral arms or prominent dust lanes. Some subtle color variations are present, perhaps indicating areas of varying stellar populations or dust concentration within the disk. The overall shape of the galaxy appears relatively undisturbed, without obvious signs of ongoing major mergers or tidal interactions.
