The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The central region exhibits a yellowish hue, possibly indicating an older stellar population. Moving outwards from the core, the galaxy appears more diffuse and blueish, suggesting a relatively low level of recent star formation compared to its overall mass. There are no clearly defined spiral arms or a prominent disk structure, but a very faint, irregular, disk-like structure may be present. There is little evidence of any major disturbances or ongoing mergers. The overall shape is somewhat elliptical.
