The galaxy presents with a bright, relatively compact core. It appears to exhibit signs of disturbance in its morphology, possibly indicating a past or ongoing interaction. There is a suggestion of tidal features, although subtle, extending from the main body of the galaxy. These features could be remnants of a minor merger event. The overall color profile suggests the presence of a younger stellar population, particularly in the central region, as well as within the outer disturbed area. There is no clear spiral structure. The galaxy appears to be experiencing some form of disruption to its overall morphology.
