The galaxy presents a predominantly smooth morphology, with a notable absence of well-defined spiral arms or prominent features. The light distribution is centrally concentrated, appearing brightest at the core and gradually fading outwards towards the edges. It exhibits a slightly elongated shape. The galaxy appears relatively isolated, with no obvious signs of major mergers. There might be some subtle disturbances, indicating a minor interaction. The colour gradient indicates a possible aging stellar population. The central region is yellow, suggesting older stars, with the outer regions presenting a slightly bluer hue, indicative of younger stars.
