The galaxy presents as a somewhat elliptical object with a smooth, concentrated central bulge. The light is dominated by yellow and red wavelengths, suggesting an older stellar population and reduced star formation. There's little evidence of significant spiral arm structure or prominent dust lanes. The overall morphology indicates that this galaxy is likely an early-type galaxy, possibly an elliptical or lenticular galaxy transitioning from a spiral. There may be some disturbance within the galaxy as seen by slight deformations of its outer edges. There is no current major merging event occuring, though some past event may be responsible for the galaxy's current shape.
