The galaxy appears as a somewhat smooth, centrally concentrated object. It exhibits a generally rounded morphology, with a slight elongation or departure from perfect circularity. The galaxy presents a dominant central bulge that is subtly brighter and more compact than its surrounding regions. This central region is characterized by a relatively smooth, diffuse light distribution. Hints of bluer colors near the center may be indicative of on-going star formation. There also appears to be some minor distortions around the edges, which may indicate a small degree of tidal interaction with another galaxy. The edges of the galaxy appear diffuse and lack a sharp boundary, suggesting a gradual decrease in stellar density with increasing distance from the galactic center.
