The galaxy presents as a relatively smooth, centrally concentrated object. The light is more concentrated toward the center, with a color that appears to be trending towards yellow, suggestive of an older stellar population. The outer regions of the galaxy fade gradually into the background, lacking distinct spiral arms or other clear features. Overall, the galaxy's morphology indicates a possible elliptical or lenticular classification, with little evidence of ongoing major star formation or significant disturbances. There might be faint traces of a disk component, but the dominant impression is of a spheroid-shaped structure.
