The galaxy presents a relatively smooth morphology overall, though with some evidence of disturbed features or a disk-like structure. The central region exhibits an elongated shape with an intermediate roundness, leaning toward a cigar-like appearance.

There are brighter concentrations of light in the central region that might be regions of star formation. These regions contribute to its absolute magnitude, suggesting ongoing stellar activity.

There is evidence of a possible minor disturbance or a merging event.
