The galaxy exhibits an overall smooth morphology, appearing largely featureless. Its shape is predominantly round, with a slight deviation toward being an elliptical form. The light distribution appears centrally concentrated with a diffuse halo, suggesting a significant bulge component. There is no obvious spiral structure, and little evidence of dust lanes within the galaxy's disk. Overall, the galaxy is a relatively bright object, emitting strongly across the visible spectrum. There may be indications of minor disturbances or asymmetries in the outer regions of the halo, although the image resolution limits detailed analysis. The color is somewhat blue, which indicates that the object is undergoing star formation. This also means that the galaxy could be a spiral galaxy, and the lack of spirals can be attributed to image quality.
