The galaxy appears to be a disk galaxy, although without clear spiral arm structure. Its overall morphology is somewhat amorphous. A bright, centrally concentrated region is observed. The color of the central region is consistent with a relatively high stellar population density. A fainter, extended disk is seen surrounding the central bulge, with some areas indicating the presence of younger stellar populations. There are indications of minor disturbances. While appearing largely isolated, there is a potential indication of gravitational interaction with a nearby galaxy. Overall, the galaxy shows characteristics of a normal disk galaxy with some signs of potential past interaction.
