The galaxy presents as a relatively smooth, elliptical-like structure. The core region exhibits a bright, concentrated luminosity, indicative of a high stellar density. A noticeable decrease in luminosity is observed as we move outward from the core, with a gradual fading into the background.

The overall color appears reddish-yellow, suggesting a population of older stars and a lower rate of recent star formation. There appears to be some slight irregularities on the edge of the galaxy, possibly due to minor gravitational interaction. Overall, the galaxy presents a rounded morphology with no distinct spiral arms or bar features clearly visible.
