The galaxy presents a generally smooth morphology with little to no apparent spiral structure or distinct features. It appears as a single concentrated luminous region, with a centrally concentrated light profile gradually diminishing outwards. The shape is somewhat elliptical, with a slight elongation. The dominant color is a yellow-red hue, suggestive of an older stellar population and relatively low rates of current star formation. There may be some minor disturbances evident, but its general features suggest it is not currently undergoing a major merger event. Overall, the galaxy appears to be a relatively evolved system.
