The galaxy presents a generally smooth appearance, exhibiting a high degree of central concentration. It appears largely spheroidal in shape, with the suggestion of a faint, extended disk component. The color profile suggests a relatively old stellar population. However, there's some evidence of ongoing star formation at the center, as evidenced by the bluer color and the presence of some dust. The image is consistent with a galaxy that has largely ceased its major star-forming activity, but may be experiencing a low level of star formation in its central regions. It is not currently undergoing a major merging event, though there may be a minor interaction or disturbance visible.
