The galaxy presents as a singular, fairly smooth object with a concentrated central bulge. The morphology suggests it is most likely an elliptical galaxy, or possibly a lenticular galaxy given the slight elongation. Its color is predominantly yellow, indicative of an older stellar population with minimal recent star formation. There appears to be some possible minor disturbances in its structure, potentially hinting at a past or ongoing minor merger event. The overall roundness suggests it is not a highly inclined spiral galaxy. The galaxy appears relatively undisturbed, with no major signs of tidal tails or significant distortions in its shape. There are hints of a faint redder area that seems to extend downward from the main galaxy body. Further observation is needed to ascertain the true cause of these disturbances.
