The galaxy presents as a disk galaxy, observed at a nearly edge-on orientation. There is a central bulge that exhibits a relatively smooth, concentrated luminosity profile, suggesting a high stellar density, with a yellow hue indicating an older stellar population. Emanating outwards are what appears to be disturbances, suggesting either interactions with another galaxy or recent mergers. These disturbances make it difficult to discern the underlying galactic structure, but hint at potentially recent episodes of significant gravitational influence. The extent of the galaxy appears to be several thousands of parsecs in diameter. The disk itself is seen to have blue regions, indicative of star formation.
