The observed galaxy presents as a relatively faint, elongated structure, likely a disk galaxy viewed at an oblique angle. A prominent, bright central bulge dominates the core, exhibiting a smooth, concentrated light distribution. Extending outwards from the bulge are fainter, diffuse regions which could possibly be spiral arms or a disk structure. The texture of these outer regions appears somewhat patchy and flocculent, suggesting the presence of stellar populations or dust obscuration. There appears to be some disturbance to the morphology of the galaxy suggesting there might have been a minor merger. There appears to be low levels of star formation within the galaxy, which is mostly contained within the disk of the galaxy. The overall color index implies a mixed stellar population, with a dominant population of older stars in the bulge, surrounded by disk stars.
