This galaxy presents a predominantly elliptical morphology, appearing cigar-shaped with a smooth texture and a slight disk feature. The central region exhibits a bright, concentrated yellowish core, possibly indicative of an older stellar population. The outer regions display a less intense, slightly bluer hue, suggesting the potential presence of a younger stellar population or some level of ongoing star formation, though at a low rate. There's no clear evidence of a major ongoing merger, though subtle disturbances cannot be ruled out. The overall structure appears relatively undisturbed. The galaxy is of intermediate size, with an apparent extent of a few arcseconds.
