The galaxy appears as a single, relatively smooth concentration of light. Its overall shape is generally round, exhibiting a slight ellipticity. There are no distinct spiral arms or a prominent disk structure visible; the light is diffuse. The galaxy exhibits a color gradient, transitioning from a yellowish-green center to a redder hue towards its outer regions. This may indicate a difference in stellar populations or dust content across the galaxy's body. There is no obvious evidence of ongoing major mergers or significant tidal disturbances affecting its structure, or other types of asymmetries.
