The galaxy appears to be an elliptical type, exhibiting a smooth, relatively featureless morphology. Its shape is elongated, approaching a cigar-like appearance. The central region displays a concentration of light, suggesting a prominent galactic nucleus. The overall color is slightly redder, consistent with an older stellar population and minimal ongoing star formation. No distinct spiral arms or dust lanes are discernible. There is no obvious evidence of any major disturbances or merging events. The galaxy has a consistent light profile fading out gradually from the center.
