The galaxy presents as a relatively smooth, elongated structure, suggesting it may be an elliptical or lenticular galaxy viewed at an angle. The central region exhibits a higher concentration of light, indicating the presence of a galactic bulge. The color is generally yellowish, possibly indicating an older stellar population and a lower rate of current star formation. There are no distinct spiral arms or prominent dust lanes visible in the image, further suggesting a lack of active star formation. The galaxy appears to be relatively isolated, with no immediately apparent signs of major ongoing mergers or tidal disturbances. However, the shape appears slightly disturbed on the left, indicating there may have been a minor merger in the past.
