The galaxy presents as a slightly flattened spheroid with a concentrated central bulge. The core appears bright and yellow-white, potentially indicating an older stellar population. Fainter bluish regions surround the central bulge, possibly indicating more recent star formation. There may be a hint of a disk structure, but it isn't sharply defined. There is some indication of minor disturbances in the structure, it doesn't appear completely relaxed. The overall appearance suggests an intermediate-mass galaxy with ongoing, but potentially declining, star formation.
