The galaxy presents a somewhat elliptical morphology, though not perfectly spherical. It exhibits a noticeable central bulge, which appears to be a relatively smooth distribution of stars.  Moving outward from the core, a fainter, disk-like structure is suggested. The colors are relatively uniform, indicating older stellar populations. There is some indication of faint spiral arms, but these features are not very distinct. The galaxy does not appear to be undergoing any major merging events, but there are some features that could be interpreted as minor disturbances in its structure.
