The galaxy appears as a moderately bright, compact object with a relatively smooth morphology. It exhibits a slightly elongated, elliptical shape, deviating subtly from a perfectly circular form. The color profile suggests a redder hue, potentially indicative of an older stellar population or significant dust content. There are no distinct spiral arms or prominent features visible, suggesting it is likely an early-type galaxy. The galaxy does not show any obvious signs of ongoing mergers or major disturbances in its overall structure.
