The observed galaxy presents as a roughly circular, relatively smooth object. Its core exhibits a strong concentration of light, appearing bright and yellowish-white in color, suggestive of an older stellar population. There is some asymmetry in its light distribution. A slight extension or tidal feature is visible, oriented below the main body. This feature is redder, indicating either dust obscuration or an older stellar population. Overall, the galaxy lacks significant features like spiral arms or dust lanes, and displays a relatively smooth morphology. There may be evidence of an interaction or merger event, due to the asymmetric morphology.