The galaxy presents as a relatively smooth, elongated spheroid. Its core region exhibits a bright, concentrated luminosity, suggesting a high stellar density. Moving outward, the light profile gradually diminishes into a faint, diffuse halo. The overall color appears slightly reddish. There is no discernible spiral structure or significant dust lane visible in this image, indicating a lack of recent major mergers or active star formation regions within the galaxy's disk, if it has one. The galaxy is significantly elongated.
