The galaxy presents as a moderately luminous, elliptical structure with a smooth, diffuse appearance. The central region exhibits a significantly higher concentration of light, suggesting a dense stellar population or possibly an active galactic nucleus, though the image resolution limits definitive determination. The galaxy appears reddish-yellow, potentially indicative of an older stellar population with a lower rate of ongoing star formation. There is a slight flattening to the elliptical shape, deviating slightly from a perfect circle. No distinct spiral arms, dust lanes, or other significant structural features are readily apparent. There's no obvious evidence of interaction or recent merger activity.
