The galaxy presents a generally smooth morphology, although there is some irregularity and potentially merging activity. The primary body of the galaxy appears somewhat elliptical in shape, but not perfectly round. The light distribution suggests that the galaxy is composed primarily of an older stellar population. There is evidence of ongoing star formation within the galaxy, as indicated by bluer regions. The galaxy appears to be undergoing some form of disturbance or interaction, potentially a minor merger event. This is suggested by the irregularity in the outer regions and a slightly elongated structure.
