The galaxy presents as a generally smooth, centrally concentrated object. It appears to be undergoing a merger or significant tidal interaction with a secondary, smaller component. The primary component exhibits a bright, yellow core, suggesting an older stellar population. The secondary component is smaller and redder in color, indicative of either a separate, redder object undergoing a merger or strong dust reddening. This galaxy appears to be in the redshift range where we often observe these types of interactions more frequently. The overall morphology suggests a relatively evolved system, possibly on the red sequence, but with ongoing interaction that could be triggering some low-level star formation. 
