The galaxy presents a relatively smooth overall appearance with an apparent slight elongation, suggesting it may be an elliptical galaxy or a lenticular galaxy viewed at a slight angle. There's a noticeable concentration of light towards the center, indicating a prominent galactic bulge. The galaxy exhibits a yellowish-orange hue, indicative of an older stellar population with less ongoing star formation. No distinct spiral arm structures are discernible. There might be a very slight disturbance visible but nothing beyond this. It appears to be a relatively massive galaxy with a low star formation rate.
