The galaxy presents as a moderately bright, somewhat elliptical or disk-like system. Its central region exhibits a concentration of yellowish light, suggesting an older stellar population and perhaps a significant bulge. The disk or extended structure shows bluer hues, indicating the presence of younger stars and ongoing star formation. The morphology appears relatively smooth, with some faint hints of spiral arm structure. The overall color is dominated by a redder spectrum, however, some regions display a more blue spectrum indicating an intermediate age and star formation activity. There is also an object to the right of the central galaxy that appears to be a companion or interacting with the primary object. No strong signs of major disturbances or a recent major merger are immediately apparent, although subtle asymmetries might indicate minor tidal interactions.
