The galaxy presents as a relatively compact object with a smooth, diffuse morphology. Its shape is broadly elliptical but deviates slightly from a perfect ellipse, exhibiting a mild elongation. There is a subtle central concentration of light, although a distinct, bright nucleus is not apparent. The color appears to be relatively uniform across the galaxy, with a slight redder tint, suggesting an older stellar population with diminished star formation. There is no evidence of spiral arm structure, dust lanes, or significant ongoing merger activity within the limits of the image resolution. Small hint of possible tidal disturbance.
