The galaxy presents a generally smooth morphology with a slight elongation. It exhibits a color profile that is redder overall, suggesting an older stellar population. There is no apparent spiral structure or distinct features like prominent dust lanes or star-forming regions visible in the image. The overall appearance is consistent with an elliptical or lenticular galaxy at a considerable distance. There's a slight asymmetry, potentially indicating a minor interaction or disturbance, however the evidence for this is minimal. The color and smoothness indicate that this is likely a more evolved galaxy with a relatively low star formation rate.