The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a concentrated, bright, yellowish hue, suggestive of an older stellar population. The outer regions display a gradual decrease in luminosity and a slightly redder color. There is a lack of prominent spiral arm structures or dust lanes visible. Its overall shape is between round and oblong, suggesting it is not perfectly spherical, but also not extremely elongated. There are no obvious signs of recent major merger activity or significant tidal disturbances, although a minor interaction cannot be entirely ruled out. Based on the observed color and morphology, the galaxy appears to be a relatively evolved system with a low rate of ongoing star formation.
