The galaxy presents a smooth, largely featureless morphology. It appears highly rounded in shape. The light is concentrated in a central bulge, which appears to be a yellowish-orange hue, suggesting an older stellar population. There is little evidence of spiral arms or significant dust lanes within the galaxy itself. Overall, the galaxy appears relatively undisturbed, with no visible signs of ongoing major mergers or tidal interactions. The light falls off fairly smoothly from the center, indicating a lack of recent major star formation events.
