The galaxy appears as a relatively smooth, elliptical object. The central region exhibits a higher luminosity, suggesting a concentrated nucleus or bulge. The overall color profile indicates a redder hue, hinting at an older stellar population with a lower rate of on-going star formation. There may be very faint hints of a disk-like structure, though the galaxy seems more likely to be elliptical. The galaxy does not display any obvious signs of major disturbances from mergers.
