The galaxy appears to be relatively compact, exhibiting a centrally concentrated luminosity profile. The overall morphology seems predominantly smooth with a bright central bulge. There is a slight hint of extended structure around the central region, however, there is some artifacting. It exhibits a blue hue, suggesting the presence of a relatively young stellar population and/or active star formation. There might be some faint disturbance in the structure. The source is unresolved enough to not fully rule out merging in this system.
