The galaxy presents as a relatively smooth, centrally concentrated object, with a generally elliptical morphology. The color profile appears broadly consistent across the galaxy’s body. The central region exhibits a slightly brighter luminosity than the surrounding areas, suggesting a possible nuclear bulge or concentration of older stars. There is a faint, diffuse halo extending beyond the central region, but no distinct spiral arm structures or prominent dust lanes are discernible in this image. The galaxy exhibits a redder hue, indicating a potentially older stellar population and/or significant dust content within the galaxy. No obvious signs of ongoing major merger activity are visible.
