The galaxy presents a primarily smooth morphology, appearing largely featureless at this resolution. It exhibits a concentrated, somewhat elliptical shape with a high degree of roundness. The color profile suggests an older stellar population, with a dominant yellowish-orange hue concentrated toward the center. There is no clear evidence of spiral arm structure or significant dust lanes. Subtle disturbances or tidal features might be present but are not clearly distinguishable. There is a possibility of a minor merger event or interaction with another galaxy influencing its shape. Based on the colors present, it seems like its star formation rate is likely low.
