The galaxy appears to be a relatively compact object with a bright, concentrated central region. Its overall shape is somewhat elliptical, possibly indicative of a disk galaxy seen at an oblique angle, or a lenticular galaxy. The color distribution suggests a mix of stellar populations, with the central region appearing bluer, hinting at ongoing or recent star formation. There is a faint, diffuse halo surrounding the brighter core, which could be indicative of an older stellar population. The galaxy also shows a hint of distortion or tidal features, suggesting a possible minor interaction with another galaxy. This could also be from internal processes.
