The galaxy appears to be a relatively smooth, elliptical galaxy with a noticeable central bulge. The light distribution is centrally concentrated, with a gradual decrease in brightness towards the outer regions. The galaxy is elongated, exhibiting an intermediate ellipticity, neither perfectly spherical nor highly flattened. There are no distinct spiral arms or prominent dust lanes visible in this image, suggesting a lack of significant ongoing star formation. The dominant color appears to be a yellow-orange hue, indicating an older stellar population and minimal presence of young, blue stars. Faint, diffuse outer regions are present, extending beyond the main body of the galaxy, which may be a stellar halo. There are no obvious signs of major mergers or tidal disturbances in this image. 
