The galaxy presents as a somewhat elongated, disk-like structure. It exhibits a prominent central bulge, appearing smooth and concentrated with a yellowish hue, suggesting an older stellar population. The disk itself is visible, extending outwards from the bulge, however the spiral arms are difficult to distinguish. The color of the disk is also consistent with that of a relatively quiescent galaxy, with little evidence of ongoing, massive star formation. The overall form suggests a galaxy that is transitioning into a more spheroidal morphology. A slight disturbance in the outer disk appears, though no strong tidal features or companion galaxies are visible within the immediate vicinity, however this may still be a minor merger.
