The galaxy presents as a relatively smooth, elliptical-like structure with a yellowish hue, indicative of an older stellar population. There is minimal evidence of spiral arms or significant dust lanes. The light is centrally concentrated, with a gradual decrease in intensity towards the outer edges. The overall shape appears slightly elongated rather than perfectly circular, approaching an 'in between' roundness morphology. There are no obvious signs of a major ongoing merger, although subtle distortions suggest a possible minor interaction in its past, or that it is currently in a state of minor disturbance. The color profile suggests a lack of significant ongoing star formation.
