The galaxy presents as an elongated, elliptical structure. The central region exhibits a concentrated luminosity, suggesting a substantial stellar population and/or active galactic nucleus. The primary color appears to be a warm, yellow-orange hue, indicative of an older stellar population with fewer hot, young stars and possibly a higher dust content. A subtle blue tinge is visible in the outer regions, particularly at one end of the galaxy, suggesting the presence of some younger, hotter stars or ongoing star formation, albeit to a limited extent. Overall, the galaxy appears relatively smooth and undisturbed, with no prominent spiral arms or signs of a major merger event.
