The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is a dominant bulge component exhibiting a yellow-orange color, indicative of an older stellar population. A faint, diffuse, and somewhat irregular disk-like structure surrounds the bulge. The disk shows hints of bluer colors in certain regions, potentially signaling areas of ongoing or recent star formation. The overall shape is close to round, with no distinct spiral arms or bar structures visible. There are no signs of major tidal disturbances or merging activity, suggesting a relatively isolated evolutionary history.
