The galaxy appears as a relatively bright, elliptical-shaped object with a smooth, concentrated light distribution. The core region displays a yellowish hue, indicative of an older stellar population. The lack of distinct spiral arms or prominent dust lanes suggests a classification towards the elliptical end of the Hubble sequence. There is evidence of a possible minor disturbance, with some asymmetry in the outer halo. A smaller, fainter object is in close proximity to the primary galaxy. The colours suggest that the galaxy is a large and relatively inactive galaxy.
