The galaxy appears as a somewhat diffuse, elliptical object with a central concentration of light. The main body exhibits a yellowish-orange hue, suggesting an older stellar population. There is a region of blue-ish tint extending outwards on one side, which could indicate an area of more recent star formation. Based on the overall morphology, the galaxy does not appear to possess a grand, well-defined spiral structure. There is a slight irregularity present, indicating a possibility of a minor gravitational disturbance. The galaxy's roundness is skewed away from perfect round. The galaxy is likely quite massive.
