The galaxy appears as a singular, relatively smooth object with a concentrated central bulge. Its overall morphology presents as elliptical, with a slight deviation from perfect circularity. There are no visible spiral arms or bar-like structures discernible in this image. The color gradient indicates a concentration of older stellar populations, transitioning from a yellow-orange center to a slightly bluer halo or outer region. No signs of active galactic nuclei or significant dust lanes are immediately apparent, suggesting a possible absence of recent major merger events. There is an indication of some minor disturbance in the galaxy. The galaxy's light distribution is fairly even, with some subtle variations in luminosity across its structure. There is some evidence of limited star formation activity.
