The galaxy presents as a somewhat diffuse, elongated structure. It appears to be relatively smooth, with no obvious spiral arms or strong dust lanes visible at this resolution. The overall color is a pale yellow-orange, suggestive of an older stellar population and/or dust obscuration within the galaxy. The elongated morphology suggests it may be an elliptical galaxy, viewed at an angle, or a disk galaxy viewed nearly edge-on. There is a slight concentration of light toward the center, indicating a possible galactic nucleus. There isn't any clear evidence of strong recent star formation, based on the color and lack of distinct blue regions. No signs of strong tidal disturbances or mergers are visible.
