The galaxy appears as a somewhat elongated, centrally concentrated object. Its core is characterized by a yellowish-orange hue, suggesting an older stellar population. The outer regions exhibit a more diffuse, greenish-blue tint, potentially indicating the presence of younger stars or ongoing star formation. The overall shape is relatively smooth, lacking any obvious spiral arms or prominent dust lanes. There is a slight asymmetry present, which could be indicative of a minor disturbance or interaction with a smaller companion. The galaxy presents no signs of a major merger event.
