The galaxy presents a generally amorphous morphology. It does not appear to be a classic elliptical, nor does it exhibit a clear spiral structure. The light distribution is somewhat irregular, with a brighter central region that could indicate a small bulge. Evidence suggests that this is a disc galaxy viewed at an angle.

There are also brighter spots or knots scattered throughout the galaxy, indicating potential regions of increased star formation or active galactic nuclei. The bluer hue is indicative of younger stellar populations. There is evidence of possible tidal features that may result from a recent or ongoing interaction. It shows signs of a potential merger or disturbance.
