The galaxy presents as a disk galaxy, although the disk is not clearly defined; it may be observed at a slight inclination. The central bulge is prominent, appearing largely smooth and concentrated with a bright intensity. There is a faint, diffuse halo surrounding the galaxy. Some irregularities or features are visible within the disk itself, indicating possible spiral arm structures or dust lanes. Overall the galaxy appears to have low star formation and is considered relatively small. There is no indication of active merging or major disturbances, although some minor interactions are possible given the slight irregularity of the disk. The overall color suggests a moderately evolved stellar population.
