The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge. Its color profile indicates a population of older stars, with a yellow-orange hue. No distinct spiral arms or prominent dust lanes are visible, suggesting a lack of ongoing, significant star formation. The galaxy appears to be fairly isolated with no obvious signs of a major merging event. There is a slight suggestion of a minor disturbance. Overall, the morphology aligns with a mature, relatively quiescent galaxy.
