The galaxy presents as a diffuse, somewhat amorphous structure with an overall elliptical morphology. Its light distribution appears relatively smooth, exhibiting a soft gradient from the central region outwards. There is little evidence of distinct spiral arms or a well-defined central bulge. The galaxy has a bluish hue, suggesting the presence of at least some recent or ongoing star formation. Subtle irregularities or minor disturbances are apparent in the light distribution, hinting at possible interactions or internal dynamics. The galaxy is moderately sized, taking up only a small portion of the image field. The overall impression is that of a galaxy that is either an elliptical galaxy with a young stellar population or a disturbed spiral galaxy that is being actively formed.
