The galaxy presents as a relatively compact structure with a distinct central bulge. Its morphology appears to be intermediate, showing characteristics of both spiral and elliptical galaxies, although the dominant impression is of a slightly disturbed disk galaxy. The central bulge exhibits a yellowish hue, potentially indicating an older stellar population. Fainter arms appear to emanate from the bulge, displaying subtle hints of blue, suggesting the presence of some younger, hotter stars and active star formation. Overall, the galaxy appears to be undergoing moderate levels of star formation within its disk, but a possible recent minor disturbance or interaction may be taking place that is affecting its overall structure.
