The galaxy presents as a single, centrally concentrated object, appearing relatively smooth in texture. The light distribution suggests a roughly elliptical morphology, though with a slight elongation, falling somewhere between round and cigar-shaped. There is no discernible spiral arm structure or strong evidence of a prominent disk component. Color gradients across the galaxy appear subtle, indicating a fairly uniform stellar population or dust distribution. There is no clear visual evidence of ongoing mergers or major disturbances in the galaxy's structure. The overall impression is that of a galaxy nearing quiescence, without significant current star formation activity.
