The galaxy appears as a faint, elongated structure with a relatively smooth profile. There is no apparent spiral arm structure visible, and the light distribution is concentrated towards the center, suggesting a significant bulge component. The galaxy's color is generally consistent throughout, with a slight shift towards redder wavelengths, which could indicate an older stellar population. The overall morphology is suggestive of an elliptical galaxy or possibly a lenticular galaxy seen edge-on, with no signs of active star formation regions or prominent dust lanes discernable in the image. There appears to be a slight asymmetry at one end, though this does not suggest a major merger event.
