The galaxy appears as a moderately bright, relatively compact object. It presents a generally smooth morphology, lacking any prominent spiral arms or a distinct central bulge. It has a slightly elliptical shape, appearing more 'in-between' than perfectly round. There is a subtle suggestion of a disk-like structure, but features are faint and not sharply defined. No significant signs of ongoing merging activity or major disturbances are apparent, although minor irregularities are visible. The color is generally consistent across the galaxy, indicating a relatively uniform stellar population with an intermediate age and star formation rate.
