The galaxy presents as a relatively smooth, centrally concentrated structure, approximately elliptical in shape, with an apparent absence of well-defined spiral arms. The galaxy displays a prominent, bright central bulge region which dominates the overall light profile. The outer regions appear fainter, and more diffuse, suggesting a gradual decline in stellar density. The color profile seems fairly uniform across the galaxy, exhibiting a bluish hue, which could indicate the presence of a moderate population of young, hot stars within the galaxy. There are some subtle irregularities that might suggest some minor disturbances, but overall the galaxy does not appear to be undergoing any major merging events.
