This galaxy exhibits a generally smooth morphology, but with potential disturbances. The galaxy appears to be comprised of diffuse light, likely from an older stellar population. The central region seems brighter and more concentrated. Hints of bluer light are present within a region of the disk, suggesting ongoing or recent star formation activity, although at a low rate. There is some evidence of a possible minor disturbance or even a merger event. This is visible in the slightly irregular shape and offset light distributions. The overall color suggests a population that is likely more evolved but with relatively low ongoing star formation. The shape is approximately round.
