The galaxy presents as a centrally concentrated, relatively smooth object with a slightly elongated morphology. Its overall color appears to be consistent with an older stellar population, exhibiting a yellowish-red hue. There is little evidence of spiral arm structure or dust lanes. The light distribution is moderately diffuse, suggesting a possible elliptical or lenticular classification, with no obvious signs of active star formation in the image. Some minimal light disturbance may be present. 
